diff --git "a/data/results/eval_random_readable_zoOLWDdW_20240716_040746/logs/log.txt" "b/data/results/eval_random_readable_zoOLWDdW_20240716_040746/logs/log.txt"
new file mode 100644--- /dev/null
+++ "b/data/results/eval_random_readable_zoOLWDdW_20240716_040746/logs/log.txt"
@@ -0,0 +1,9886 @@
+2024-07-16 04:07:46,683 - INFO - setting random seeds and environment variables...
+2024-07-16 04:07:47,224 - INFO - loading schema and data...
+2024-07-16 04:07:47,229 - INFO - Number of training examples: 3
+2024-07-16 04:07:47,230 - INFO - Number of validation examples: 17
+2024-07-16 04:07:47,230 - INFO - loading model and tokenizer...
+2024-07-16 04:19:35,060 - INFO - generating base prompt...
+2024-07-16 04:19:35,074 - INFO - running the model...
+2024-07-16 04:19:35,074 - INFO - Run type: eval
+2024-07-16 04:19:35,074 - INFO - Data: None
+2024-07-16 04:19:35,075 - INFO - Model: meta-llama/Meta-Llama-3-70B-Instruct
+2024-07-16 04:19:35,075 - INFO - Run parameters: kind=readable, temperature=0.6, top_p=0.95, few_shot_num=3, few_shot_selection=random
+2024-07-16 04:19:35,076 - INFO - ##################################################
+2024-07-16 04:19:39,298 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The radiative transfer at second order: a full treatment of the Boltzmann equation with polarization
+Extractions:
+
+
+2024-07-16 04:19:39,299 - INFO - True Tag:
+{'object': ['radiative transfer at second order'], 'method': ['Boltzmann equation']}
+
+2024-07-16 04:19:39,300 - INFO - Predicted Response:
+assistant
+
+method: radiative transfer
+
+2024-07-16 04:19:39,300 - INFO - Predicted Tag:
+{'method': ['radiative transfer']}
+
+2024-07-16 04:19:41,276 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: This article investigates the full Boltzmann equation up to second order in the cosmological perturbations
+Extractions:
+
+
+2024-07-16 04:19:41,276 - INFO - True Tag:
+{'method': ['Boltzmann equation'], 'object': ['cosmological perturbations'], 'field': ['cosmological']}
+
+2024-07-16 04:19:41,276 - INFO - Predicted Response:
+assistant
+
+model: Boltzmann equation
+
+2024-07-16 04:19:41,276 - INFO - Predicted Tag:
+{'model': ['Boltzmann equation']}
+
+2024-07-16 04:19:44,875 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Describing the distribution of polarized radiation by a tensor valued distribution function, we study the gauge dependence of the distribution function and summarize the construction of the gauge-invariant distribution function
+Extractions:
+
+
+2024-07-16 04:19:44,875 - INFO - True Tag:
+{'object': ['polarized radiation'], 'method': ['tensor valued distribution function', 'distribution function', 'gauge-invariant distribution function'], 'property': ['gauge dependence', 'gauge-invariant']}
+
+2024-07-16 04:19:44,875 - INFO - Predicted Response:
+assistant
+
+model: tensor valued distribution function, gauge-invariant distribution function
+object: polarized radiation, distribution function
+
+2024-07-16 04:19:44,876 - INFO - Predicted Tag:
+{'model': ['tensor valued distribution function', 'gauge-invariant distribution function'], 'object': ['polarized radiation', 'distribution function']}
+
+2024-07-16 04:19:47,178 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The Liouville operator which describes the free streaming of electrons, and the collision term which describes the scattering of photons on free electrons are computed up to second order
+Extractions:
+
+
+2024-07-16 04:19:47,178 - INFO - True Tag:
+{'model': ['Liouville operator'], 'object': ['electrons', 'collision term', 'scattering of photons', 'free electrons']}
+
+2024-07-16 04:19:47,178 - INFO - Predicted Response:
+assistant
+
+method: Liouville operator, collision term
+
+2024-07-16 04:19:47,178 - INFO - Predicted Tag:
+{'method': ['Liouville operator', 'collision term']}
+
+2024-07-16 04:19:49,485 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Finally, the remaining dependence in the direction of the photon momentum is handled by expanding in projected symmetric trace-free multipoles and also in the more commonly used normal modes components
+Extractions:
+
+
+2024-07-16 04:19:49,485 - INFO - True Tag:
+{'property': ['dependence', 'momentum', 'symmetric', 'trace-free'], 'object': ['photon', 'multipoles', 'normal modes components']}
+
+2024-07-16 04:19:49,485 - INFO - Predicted Response:
+assistant
+
+modality: multipoles, normal modes
+
+2024-07-16 04:19:49,485 - INFO - Predicted Tag:
+{'modality': ['multipoles', 'normal modes']}
+
+2024-07-16 04:19:52,774 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The results obtained remain to be used for computing numerically the contribution in the cosmic microwave background bispectrum which arises from the evolution of second order perturbations, in order to disentangle the primordial non-Gaussianity from the one generated by the subsequent non-linear evolution.
+Extractions:
+
+
+2024-07-16 04:19:52,774 - INFO - True Tag:
+{'object': ['cosmic microwave background bispectrum', 'second order perturbations', 'non-linear evolution'], 'property': ['bispectrum', 'primordial non-Gaussianity', 'non-linear']}
+
+2024-07-16 04:19:52,774 - INFO - Predicted Response:
+assistant
+
+model: cosmic microwave background
+object: perturbations, non-Gaussianity, evolution
+
+2024-07-16 04:19:52,774 - INFO - Predicted Tag:
+{'model': ['cosmic microwave background'], 'object': ['perturbations', 'non-Gaussianity', 'evolution']}
+
+2024-07-16 04:19:52,774 - INFO - ##################################################
+2024-07-16 04:19:54,955 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Independent confirmation and refined parameters of the hot Jupiter XO-5b
+Extractions:
+
+
+2024-07-16 04:19:54,955 - INFO - True Tag:
+{'object': ['Jupiter XO-5b']}
+
+2024-07-16 04:19:54,955 - INFO - Predicted Response:
+assistant
+
+object: XO-5b, Jupiter
+
+2024-07-16 04:19:54,955 - INFO - Predicted Tag:
+{'object': ['XO-5b', 'Jupiter']}
+
+2024-07-16 04:19:58,013 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We present HATNet observations of XO-5b, confirming its planetary nature based on evidence beyond that described in the announcement of Burke et al
+Extractions:
+
+
+2024-07-16 04:19:58,014 - INFO - True Tag:
+{'dataset': ['HATNet observations'], 'instrument': ['HATNet'], 'object': ['XO-5b']}
+
+2024-07-16 04:19:58,014 - INFO - Predicted Response:
+assistant
+
+dataset: HATNet observations
+object: XO-5b, planetary nature
+
+2024-07-16 04:19:58,014 - INFO - Predicted Tag:
+{'dataset': ['HATNet observations'], 'object': ['XO-5b', 'planetary nature']}
+
+2024-07-16 04:20:00,310 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: (2008), namely, the lack of significant correlation between spectral bisector variations and orbital phase
+Extractions:
+
+
+2024-07-16 04:20:00,310 - INFO - True Tag:
+{'property': ['correlation', 'spectral bisector variations', 'orbital phase']}
+
+2024-07-16 04:20:00,310 - INFO - Predicted Response:
+assistant
+
+property: spectral bisector variations, orbital phase
+
+2024-07-16 04:20:00,310 - INFO - Predicted Tag:
+{'property': ['spectral bisector variations', 'orbital phase']}
+
+2024-07-16 04:20:02,180 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In addition, using extensive spectroscopic measurements spanning multiple seasons, we investigate the relatively large scatter in the spectral line bisectors
+Extractions:
+
+
+2024-07-16 04:20:02,180 - INFO - True Tag:
+{'modality': ['spectroscopic measurements'], 'property': ['scatter', 'spectral line bisectors']}
+
+2024-07-16 04:20:02,180 - INFO - Predicted Response:
+assistant
+
+dataset: spectroscopic measurements
+
+2024-07-16 04:20:02,180 - INFO - Predicted Tag:
+{'dataset': ['spectroscopic measurements']}
+
+2024-07-16 04:20:04,596 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We also examine possible blended stellar configurations (hierarchical triples, chance alignments) that can mimic the planet signals, and we are able to show that none are consistent with the sum of all the data
+Extractions:
+
+
+2024-07-16 04:20:04,597 - INFO - True Tag:
+{'object': ['stellar configurations', 'hierarchical triples', 'chance alignments', 'planet signals']}
+
+2024-07-16 04:20:04,597 - INFO - Predicted Response:
+assistant
+
+Extractions:
+object: planet signals, data
+
+2024-07-16 04:20:04,597 - INFO - Predicted Tag:
+{'object': ['planet signals', 'data']}
+
+2024-07-16 04:20:06,783 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The analysis of the S activity index shows no significant stellar activity
+Extractions:
+
+
+2024-07-16 04:20:06,783 - INFO - True Tag:
+{'property': ['S activity index'], 'object': ['stellar activity']}
+
+2024-07-16 04:20:06,783 - INFO - Predicted Response:
+assistant
+
+object: S activity index, stellar activity
+
+2024-07-16 04:20:06,783 - INFO - Predicted Tag:
+{'object': ['S activity index', 'stellar activity']}
+
+2024-07-16 04:20:08,539 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Our results for the planet parameters are consistent with values in Burke et al
+Extractions:
+
+
+2024-07-16 04:20:08,539 - INFO - True Tag:
+{'object': ['planet parameters']}
+
+2024-07-16 04:20:08,539 - INFO - Predicted Response:
+assistant
+
+object: planet parameters
+
+2024-07-16 04:20:08,539 - INFO - Predicted Tag:
+{'object': ['planet parameters']}
+
+2024-07-16 04:20:10,294 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: (2008), and we refine both the stellar and planetary parameters using our data
+Extractions:
+
+
+2024-07-16 04:20:10,294 - INFO - True Tag:
+{'object': ['stellar and planetary parameters']}
+
+2024-07-16 04:20:10,294 - INFO - Predicted Response:
+assistant
+
+No extractions.
+
+2024-07-16 04:20:10,294 - INFO - Predicted Tag:
+{}
+
+2024-07-16 04:20:13,467 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: XO-5b orbits a slightly evolved, late G type star with mass M_s = 0.88 +/- 0.03, radius R_s = 1.08 +/- 0.04, and metallicity close to solar
+Extractions:
+
+
+2024-07-16 04:20:13,467 - INFO - True Tag:
+{'object': ['XO-5b', 'G type star'], 'property': ['mass', 'M_s', 'radius', 'R_s', 'metallicity']}
+
+2024-07-16 04:20:13,467 - INFO - Predicted Response:
+assistant
+
+object: XO-5b, star
+property: mass, radius, metallicity
+
+2024-07-16 04:20:13,467 - INFO - Predicted Tag:
+{'object': ['XO-5b', 'star'], 'property': ['mass', 'radius', 'metallicity']}
+
+2024-07-16 04:20:16,221 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The planetary mass and radius are M_p = 1.059 +/- 0.028 M_Jup and R_p = 1.109 +/- 0.050 R_Jup, respectively, corresponding to a mean density of 0.96 -0.11 +0.14 g/cm^3
+Extractions:
+
+
+2024-07-16 04:20:16,221 - INFO - True Tag:
+{'property': ['mass', 'radius', 'M_p', 'R_p', 'mean density']}
+
+2024-07-16 04:20:16,221 - INFO - Predicted Response:
+assistant
+
+property: planetary mass, radius, mean density
+object: planet
+
+2024-07-16 04:20:16,221 - INFO - Predicted Tag:
+{'property': ['planetary mass', 'radius', 'mean density'], 'object': ['planet']}
+
+2024-07-16 04:20:18,430 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The ephemeris for the orbit is P = 4.187757 +/- 0.000011, E= 2454552.67168 +/- 0.00029 (BJD) with transit duration of 0.1307 +/- 0.0013 d
+Extractions:
+
+
+2024-07-16 04:20:18,430 - INFO - True Tag:
+{'property': ['ephemeris', 'orbit', 'P', 'E', 'transit duration']}
+
+2024-07-16 04:20:18,430 - INFO - Predicted Response:
+assistant
+
+property: P, E, transit duration
+
+2024-07-16 04:20:18,430 - INFO - Predicted Tag:
+{'property': ['P', 'E', 'transit duration']}
+
+2024-07-16 04:20:20,292 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: By measuring four individual transit centers, we found no signs for transit timing variations
+Extractions:
+
+
+2024-07-16 04:20:20,292 - INFO - True Tag:
+{'object': ['transit timing variations']}
+
+2024-07-16 04:20:20,292 - INFO - Predicted Response:
+assistant
+
+property: transit timing variations
+
+2024-07-16 04:20:20,292 - INFO - Predicted Tag:
+{'property': ['transit timing variations']}
+
+2024-07-16 04:20:23,895 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The planet XO-5b is notable for its anomalously high Safronov number, and has a high surface gravity when compared to other transiting exoplanets with similar period.
+Extractions:
+
+
+2024-07-16 04:20:23,895 - INFO - True Tag:
+{'object': ['XO-5b', 'exoplanets'], 'property': ['Safronov number', 'gravity']}
+
+2024-07-16 04:20:23,895 - INFO - Predicted Response:
+assistant
+
+object: XO-5b, exoplanets
+property: Safronov number, surface gravity
+
+2024-07-16 04:20:23,895 - INFO - Predicted Tag:
+{'object': ['XO-5b', 'exoplanets'], 'property': ['Safronov number', 'surface gravity']}
+
+2024-07-16 04:20:23,896 - INFO - ##################################################
+2024-07-16 04:20:26,188 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Electron Temperatures in W51 Complex from High Resolution, Low Frequency Radio Observations
+Extractions:
+
+
+2024-07-16 04:20:26,188 - INFO - True Tag:
+{'property': ['Electron Temperatures', 'High Resolution', 'Low Frequency'], 'object': ['W51 Complex'], 'modality': ['Radio']}
+
+2024-07-16 04:20:26,188 - INFO - Predicted Response:
+assistant
+
+object: Electron Temperatures, W51 Complex
+
+2024-07-16 04:20:26,188 - INFO - Predicted Tag:
+{'object': ['Electron Temperatures', 'W51 Complex']}
+
+2024-07-16 04:20:29,362 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: W51 is a giant radio complex lying along the tangent to the Sagitarius arm at a distance of about 7kpc from Sun, with an extension of about 1deg in the sky
+Extractions:
+
+
+2024-07-16 04:20:29,362 - INFO - True Tag:
+{'object': ['W51', 'radio complex', 'Sagitarius arm', 'Sun'], 'modality': ['radio']}
+
+2024-07-16 04:20:29,362 - INFO - Predicted Response:
+assistant
+
+object: W51, Sagitarius arm, Sun 
+property: distance, extension
+
+2024-07-16 04:20:29,362 - INFO - Predicted Tag:
+{'object': ['W51', 'Sagitarius arm', 'Sun '], 'property': ['distance', 'extension']}
+
+2024-07-16 04:20:33,071 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: It is divided into three components A,B,C where W51A and W51B consist of many compact HII regions while W51C is a supernova remnant
+Extractions:
+
+
+2024-07-16 04:20:33,071 - INFO - True Tag:
+{'object': ['W51A', 'W51B', 'HII regions', 'W51C', 'supernova remnant']}
+
+2024-07-16 04:20:33,071 - INFO - Predicted Response:
+assistant
+
+object: W51A, W51B, W51C, HII regions, supernova remnant
+
+2024-07-16 04:20:33,071 - INFO - Predicted Tag:
+{'object': ['W51A', 'W51B', 'W51C', 'HII regions', 'supernova remnant']}
+
+2024-07-16 04:20:37,116 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We have made continuum radio observations of these HII regions of the W51 complex at 240,610,1060,1400 MHz using GMRT with lower resolution 20''x15'' at the lowest frequency
+Extractions:
+
+
+2024-07-16 04:20:37,116 - INFO - True Tag:
+{'dataset': ['continuum radio observations'], 'modality': ['continuum radio'], 'object': ['HII regions', 'W51'], 'instrument': ['GMRT']}
+
+2024-07-16 04:20:37,116 - INFO - Predicted Response:
+assistant
+
+dataset: continuum radio observations
+instrument: GMRT
+modality: radio
+object: HII regions, W51 complex
+
+2024-07-16 04:20:37,116 - INFO - Predicted Tag:
+{'dataset': ['continuum radio observations'], 'instrument': ['GMRT'], 'modality': ['radio'], 'object': ['HII regions', 'W51 complex']}
+
+2024-07-16 04:20:40,720 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The observed spectra of the prominent thermal subcomponents of W51 have been fitted to a free-free emission spectrum and their physical properties like electron temperatures and emission measures have been estimated
+Extractions:
+
+
+2024-07-16 04:20:40,720 - INFO - True Tag:
+{'modality': ['spectra'], 'property': ['thermal subcomponents', 'electron temperatures', 'emission measures'], 'object': ['W51', 'emission spectrum']}
+
+2024-07-16 04:20:40,720 - INFO - Predicted Response:
+assistant
+
+object: W51, thermal subcomponents
+property: electron temperatures, emission measures
+modality: spectra
+
+2024-07-16 04:20:40,720 - INFO - Predicted Tag:
+{'object': ['W51', 'thermal subcomponents'], 'property': ['electron temperatures', 'emission measures'], 'modality': ['spectra']}
+
+2024-07-16 04:20:44,759 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The electron temperatures from continuum spectra are found to be lower than the temperatures reported from radio recombination line (RRL) studies of these HII regions indicating the need for a filling factor even at this resolution
+Extractions:
+
+
+2024-07-16 04:20:44,759 - INFO - True Tag:
+{'property': ['electron temperatures', 'temperatures'], 'modality': ['continuum spectra'], 'method': ['radio recombination line (RRL) studies'], 'object': ['HII regions']}
+
+2024-07-16 04:20:44,759 - INFO - Predicted Response:
+assistant
+
+instrument: continuum spectra, radio recombination line (RRL)
+modality: spectra
+property: electron temperatures, filling factor
+
+2024-07-16 04:20:44,759 - INFO - Predicted Tag:
+{'instrument': ['continuum spectra', 'radio recombination line (RRL)'], 'modality': ['spectra'], 'property': ['electron temperatures', 'filling factor']}
+
+2024-07-16 04:20:46,742 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Also, the observed brightness at 240MHz is found to be higher than expected from the best fits suggesting the need for a multicomponent model for the region.
+Extractions:
+
+
+2024-07-16 04:20:46,742 - INFO - True Tag:
+{'property': ['brightness'], 'model': ['multicomponent model']}
+
+2024-07-16 04:20:46,742 - INFO - Predicted Response:
+assistant
+
+model: multicomponent model
+
+2024-07-16 04:20:46,742 - INFO - Predicted Tag:
+{'model': ['multicomponent model']}
+
+2024-07-16 04:20:46,771 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746
+2024-07-16 04:20:46,771 - INFO - ##################################################
+2024-07-16 04:20:50,047 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Dynamical Study of A1689 from Wide-Field VLT/VIMOS Spectroscopy: Mass Profile, Concentration Parameter, and Velocity Anisotropy
+Extractions:
+
+
+2024-07-16 04:20:50,047 - INFO - True Tag:
+{'object': ['A1689', 'Wide-Field VLT/VIMOS Spectroscopy'], 'instrument': ['VLT/VIMOS'], 'modality': ['Spectroscopy'], 'property': ['Mass Profile', 'Concentration Parameter', 'Velocity Anisotropy']}
+
+2024-07-16 04:20:50,047 - INFO - Predicted Response:
+assistant
+
+object: A1689, Mass Profile, Concentration Parameter, Velocity Anisotropy
+
+2024-07-16 04:20:50,047 - INFO - Predicted Tag:
+{'object': ['A1689', 'Mass Profile', 'Concentration Parameter', 'Velocity Anisotropy']}
+
+2024-07-16 04:20:55,813 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We examine the dynamics structure of the rich cluster A1689, combining VLT/VIMOS spectroscopy with Subaru/Suprime-Cam imaging
+Extractions:
+
+
+2024-07-16 04:20:55,813 - INFO - True Tag:
+{'object': ['cluster A1689'], 'modality': ['VLT/VIMOS spectroscopy', 'Subaru/Suprime-Cam imaging'], 'instrument': ['VLT/VIMOS', 'Subaru/Suprime-Cam']}
+
+2024-07-16 04:20:55,813 - INFO - Predicted Response:
+assistant
+
+dataset: VLT/VIMOS spectroscopy, Subaru/Suprime-Cam imaging
+instrument: VLT/VIMOS, Subaru/Suprime-Cam
+object: cluster A1689
+
+2024-07-16 04:20:55,813 - INFO - Predicted Tag:
+{'dataset': ['VLT/VIMOS spectroscopy', 'Subaru/Suprime-Cam imaging'], 'instrument': ['VLT/VIMOS', 'Subaru/Suprime-Cam'], 'object': ['cluster A1689']}
+
+2024-07-16 04:20:59,446 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The radial velocity distribution of $\sim 500$ cluster members is bounded by a pair of clearly defined velocity caustics, with a maximum amplitude of $\sim|4000|$ km/s at $\simeq$ 300 h$^{-1}$ kpc, beyond which the amplitude steadily declines, approaching zero velocity at a limiting radius of $\sim$ 2 h$^{-1}$ Mpc
+Extractions:
+
+
+2024-07-16 04:20:59,446 - INFO - True Tag:
+{'property': ['radial velocity distribution', 'amplitude', 'radius'], 'object': ['cluster members']}
+
+2024-07-16 04:20:59,446 - INFO - Predicted Response:
+assistant
+
+property: radial velocity distribution, amplitude, velocity, radius
+object: cluster members, velocity caustics
+
+2024-07-16 04:20:59,446 - INFO - Predicted Tag:
+{'property': ['radial velocity distribution', 'amplitude', 'velocity', 'radius'], 'object': ['cluster members', 'velocity caustics']}
+
+2024-07-16 04:21:04,689 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We derive the 3D velocity anisotropy and galaxy number density profiles using a model-independent method to solve the Jeans equation, simultaneously incorporating the observed velocity dispersion profile, the galaxy counts from deep Subaru imaging, and our previously derived cluster mass profile from a joint lensing and X-ray analysis
+Extractions:
+
+
+2024-07-16 04:21:04,689 - INFO - True Tag:
+{'property': ['3D velocity anisotropy', 'galaxy number density', 'velocity dispersion', 'galaxy counts', 'cluster mass'], 'method': ['Jeans equation'], 'instrument': ['Subaru imaging'], 'modality': ['joint lensing', 'X-ray']}
+
+2024-07-16 04:21:04,689 - INFO - Predicted Response:
+assistant
+
+model: Jeans equation
+method: model-independent method
+object: velocity anisotropy, galaxy, velocity dispersion, galaxy counts, cluster mass profile
+property: 3D
+
+2024-07-16 04:21:04,689 - INFO - Predicted Tag:
+{'model': ['Jeans equation'], 'method': ['model-independent method'], 'object': ['velocity anisotropy', 'galaxy', 'velocity dispersion', 'galaxy counts', 'cluster mass profile'], 'property': ['3D']}
+
+2024-07-16 04:21:06,775 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The velocity anisotropy is found to be predominantly radial at large radius, becoming increasingly tangential towards the center, in accord with expectations
+Extractions:
+
+
+2024-07-16 04:21:06,775 - INFO - True Tag:
+{'property': ['velocity anisotropy', 'radial', 'radius']}
+
+2024-07-16 04:21:06,775 - INFO - Predicted Response:
+assistant
+
+property: velocity anisotropy
+
+2024-07-16 04:21:06,775 - INFO - Predicted Tag:
+{'property': ['velocity anisotropy']}
+
+2024-07-16 04:21:10,714 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We also analyze the galaxy data independently of our previous analysis using two different methods: The first is based on a solution of the Jeans equation assuming an NFW form for the mass distribution, whereas in the second method the caustic amplitude is used to determine the escape velocity
+Extractions:
+
+
+2024-07-16 04:21:10,715 - INFO - True Tag:
+{'object': ['galaxy'], 'method': ['Jeans equation', 'NFW form for the mass distribution'], 'property': ['caustic amplitude', 'escape velocity']}
+
+2024-07-16 04:21:10,715 - INFO - Predicted Response:
+assistant
+
+method: solution of the Jeans equation, method
+object: galaxy, mass distribution, caustic amplitude, escape velocity
+
+2024-07-16 04:21:10,715 - INFO - Predicted Tag:
+{'method': ['solution of the Jeans equation', 'method'], 'object': ['galaxy', 'mass distribution', 'caustic amplitude', 'escape velocity']}
+
+2024-07-16 04:21:14,098 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The cluster virial mass derived by both of these dynamical methods is in good agreement with results from our earlier lensing and X-ray analysis
+Extractions:
+
+
+2024-07-16 04:21:14,098 - INFO - True Tag:
+{'object': ['cluster'], 'property': ['virial mass'], 'modality': ['lensing', 'X-ray']}
+
+2024-07-16 04:21:14,098 - INFO - Predicted Response:
+assistant
+
+model: dynamical methods
+object: cluster virial mass, lensing, X-ray analysis
+
+2024-07-16 04:21:14,099 - INFO - Predicted Tag:
+{'model': ['dynamical methods'], 'object': ['cluster virial mass', 'lensing', 'X-ray analysis']}
+
+2024-07-16 04:21:16,081 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We also confirm the high NFW concentration parameter, with results from both methods combined to yield $c_{\rm vir}>13$ (1$\sigma$)
+Extractions:
+
+
+2024-07-16 04:21:16,081 - INFO - True Tag:
+{'property': ['NFW concentration parameter']}
+
+2024-07-16 04:21:16,081 - INFO - Predicted Response:
+assistant
+
+property: NFW concentration parameter
+
+2024-07-16 04:21:16,081 - INFO - Predicted Tag:
+{'property': ['NFW concentration parameter']}
+
+2024-07-16 04:21:19,578 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The inferred virial radius is consistent with the limiting radius where the caustics approach zero velocity and where the counts of cluster members drop off, suggesting that infall onto A1689 is currently not significant.
+Extractions:
+
+
+2024-07-16 04:21:19,578 - INFO - True Tag:
+{'property': ['virial radius', 'radius', 'caustics', 'velocity'], 'object': ['cluster', 'A1689']}
+
+2024-07-16 04:21:19,578 - INFO - Predicted Response:
+assistant
+
+object: virial radius, caustics, cluster members, A1689
+property: velocity
+
+2024-07-16 04:21:19,579 - INFO - Predicted Tag:
+{'object': ['virial radius', 'caustics', 'cluster members', 'A1689'], 'property': ['velocity']}
+
+2024-07-16 04:21:19,579 - INFO - ##################################################
+2024-07-16 04:21:21,979 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Systematic thermal reduction of neutronization in core-collapse supernovae
+Extractions:
+
+
+2024-07-16 04:21:21,979 - INFO - True Tag:
+{'property': ['neutronization', 'core-collapse'], 'object': ['supernovae']}
+
+2024-07-16 04:21:21,979 - INFO - Predicted Response:
+assistant
+
+object: neutronization, core-collapse supernovae
+
+2024-07-16 04:21:21,979 - INFO - Predicted Tag:
+{'object': ['neutronization', 'core-collapse supernovae']}
+
+2024-07-16 04:21:24,714 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We investigate to what extent the temperature dependence of the nuclear symmetry energy can affect the neutronization of the stellar core prior to neutrino trapping during gravitational collapse
+Extractions:
+
+
+2024-07-16 04:21:24,714 - INFO - True Tag:
+{'property': ['temperature dependence', 'neutronization'], 'object': ['nuclear symmetry energy', 'stellar core', 'neutrino', 'gravitational collapse']}
+
+2024-07-16 04:21:24,714 - INFO - Predicted Response:
+assistant
+
+property: temperature dependence, nuclear symmetry energy
+object: stellar core
+
+2024-07-16 04:21:24,714 - INFO - Predicted Tag:
+{'property': ['temperature dependence', 'nuclear symmetry energy'], 'object': ['stellar core']}
+
+2024-07-16 04:21:27,231 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: To this end, we implement a one-zone simulation to follow the collapse until beta equilibrium is reached and the lepton fraction remains constant
+Extractions:
+
+
+2024-07-16 04:21:27,232 - INFO - True Tag:
+{'method': ['one-zone simulation'], 'property': ['collapse', 'beta equilibrium'], 'object': ['lepton fraction']}
+
+2024-07-16 04:21:27,232 - INFO - Predicted Response:
+assistant
+
+model: one-zone simulation
+task: follow the collapse
+
+2024-07-16 04:21:27,232 - INFO - Predicted Tag:
+{'model': ['one-zone simulation'], 'task': ['follow the collapse']}
+
+2024-07-16 04:21:29,318 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Since the strength of electron capture on the neutron-rich nuclei associated to the supernova scenario is still an open issue, we keep it as a free parameter
+Extractions:
+
+
+2024-07-16 04:21:29,318 - INFO - True Tag:
+{'property': ['strength', 'neutron-rich'], 'object': ['electron capture', 'electron', 'nuclei', 'supernova']}
+
+2024-07-16 04:21:29,318 - INFO - Predicted Response:
+assistant
+
+Extractions:
+property: strength
+
+2024-07-16 04:21:29,318 - INFO - Predicted Tag:
+{'property': ['strength']}
+
+2024-07-16 04:21:32,520 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We find that the temperature dependence of the symmetry energy consistently yields a small reduction of deleptonization, which corresponds to a systematic effect on the shock wave energetics: the gain in dissociation energy of the shock has a small yet non-negligible value of about 0.4 foe (1 foe = 10^51 erg) and this result is almost independent from the strength of nuclear electron capture
+Extractions:
+
+
+2024-07-16 04:21:32,520 - INFO - True Tag:
+{'property': ['temperature dependence', 'dissociation energy', 'strength'], 'object': ['symmetry energy', 'deleptonization', 'shock wave energetics', 'nuclear electron capture', 'electron']}
+
+2024-07-16 04:21:32,520 - INFO - Predicted Response:
+assistant
+
+property: temperature dependence, symmetry energy, dissociation energy, shock wave energetics
+
+2024-07-16 04:21:32,520 - INFO - Predicted Tag:
+{'property': ['temperature dependence', 'symmetry energy', 'dissociation energy', 'shock wave energetics']}
+
+2024-07-16 04:21:34,395 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The presence of such a systematic effect and its robustness under changes of the parameters of the one-zone model are significative enough to justify further investigations with detailed numerical simulations of supernova explosions.
+Extractions:
+
+
+2024-07-16 04:21:34,395 - INFO - True Tag:
+{'method': ['one-zone model'], 'task': ['numerical simulations'], 'object': ['supernova explosions']}
+
+2024-07-16 04:21:34,395 - INFO - Predicted Response:
+assistant
+
+model: one-zone model
+
+2024-07-16 04:21:34,395 - INFO - Predicted Tag:
+{'model': ['one-zone model']}
+
+2024-07-16 04:21:34,395 - INFO - ##################################################
+2024-07-16 04:21:36,894 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Hadrons As Kerr-Newman Black Holes
+Extractions:
+
+
+2024-07-16 04:21:36,894 - INFO - True Tag:
+{'object': ['Hadrons', 'Kerr-Newman Black Holes']}
+
+2024-07-16 04:21:36,894 - INFO - Predicted Response:
+assistant
+
+object: Hadrons, Kerr-Newman Black Holes
+
+2024-07-16 04:21:36,894 - INFO - Predicted Tag:
+{'object': ['Hadrons', 'Kerr-Newman Black Holes']}
+
+2024-07-16 04:21:38,774 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The scale invariance of the source-free Einstein field equations suggests that one might be able to model hadrons as "strong gravity" black holes, if one uses an appropriate rescaling of units or a revised gravitational coupling factor
+Extractions:
+
+
+2024-07-16 04:21:38,774 - INFO - True Tag:
+{'property': ['scale invariance', '\\"strong gravity\\"'], 'model': ['Einstein field equations'], 'object': ['hadrons', 'black holes', 'gravitational coupling factor']}
+
+2024-07-16 04:21:38,774 - INFO - Predicted Response:
+assistant
+
+model: Einstein field equations
+
+2024-07-16 04:21:38,774 - INFO - Predicted Tag:
+{'model': ['Einstein field equations']}
+
+2024-07-16 04:21:42,053 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The inner consistency of this hypothesis is tested by retrodicting a close approximation to the mass of the proton from an equation that relates the angular momentum and mass of a Kerr black hole
+Extractions:
+
+
+2024-07-16 04:21:42,054 - INFO - True Tag:
+{'task': ['retrodicting'], 'property': ['mass', 'angular momentum'], 'object': ['proton', 'Kerr black hole']}
+
+2024-07-16 04:21:42,054 - INFO - Predicted Response:
+assistant
+
+model: hypothesis
+object: proton, Kerr black hole
+property: mass, angular momentum
+
+2024-07-16 04:21:42,054 - INFO - Predicted Tag:
+{'model': ['hypothesis'], 'object': ['proton', 'Kerr black hole'], 'property': ['mass', 'angular momentum']}
+
+2024-07-16 04:21:45,226 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: More accurate mass and radius values for the proton are then retrodicted using the geometrodynamics form of the full Kerr-Newman solution of the Einstein-Maxwell equations
+Extractions:
+
+
+2024-07-16 04:21:45,226 - INFO - True Tag:
+{'property': ['mass', 'radius'], 'object': ['proton'], 'method': ['geometrodynamics form', 'full Kerr-Newman solution'], 'model': ['Einstein-Maxwell equations']}
+
+2024-07-16 04:21:45,226 - INFO - Predicted Response:
+assistant
+
+model: Kerr-Newman solution of the Einstein-Maxwell equations
+object: proton
+
+2024-07-16 04:21:45,226 - INFO - Predicted Tag:
+{'model': ['Kerr-Newman solution of the Einstein-Maxwell equations'], 'object': ['proton']}
+
+2024-07-16 04:21:47,414 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The radius of an alpha particle is calculated as an additional retrodictive test
+Extractions:
+
+
+2024-07-16 04:21:47,414 - INFO - True Tag:
+{'property': ['radius'], 'object': ['alpha particle'], 'task': ['retrodictive test']}
+
+2024-07-16 04:21:47,414 - INFO - Predicted Response:
+assistant
+
+object: alpha particle
+property: radius
+
+2024-07-16 04:21:47,414 - INFO - Predicted Tag:
+{'object': ['alpha particle'], 'property': ['radius']}
+
+2024-07-16 04:21:50,483 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In a third retrodictive test of the "strong gravity" hypothesis, the subatomic particle mass spectrum in the 100 MeV to 7,000 MeV range is retrodicted to a first approximation using the Kerr solution of General Relativity
+Extractions:
+
+
+2024-07-16 04:21:50,484 - INFO - True Tag:
+{'task': ['retrodictive test', 'retrodicted'], 'modality': ['subatomic particle mass spectrum'], 'method': ['Kerr solution of General Relativity']}
+
+2024-07-16 04:21:50,484 - INFO - Predicted Response:
+assistant
+
+model: Kerr solution of General Relativity
+object: subatomic particle mass spectrum
+
+2024-07-16 04:21:50,484 - INFO - Predicted Tag:
+{'model': ['Kerr solution of General Relativity'], 'object': ['subatomic particle mass spectrum']}
+
+2024-07-16 04:21:53,443 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The particle masses appear to form a restricted set of quantized values of the Kerr solution: n^1/2 M, where values of n are a set of discrete integers and M is the revised Planck mass
+Extractions:
+
+
+2024-07-16 04:21:53,443 - INFO - True Tag:
+{'object': ['particle masses'], 'method': ['Kerr solution'], 'property': ['n', 'M', 'Planck mass']}
+
+2024-07-16 04:21:53,443 - INFO - Predicted Response:
+assistant
+
+property: particle masses, Kerr solution, Planck mass
+object: particle
+
+2024-07-16 04:21:53,443 - INFO - Predicted Tag:
+{'property': ['particle masses', 'Kerr solution', 'Planck mass'], 'object': ['particle']}
+
+2024-07-16 04:21:55,094 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The accuracy of the 27 retrodicted masses averages 98.4%
+Extractions:
+
+
+2024-07-16 04:21:55,094 - INFO - True Tag:
+{'object': ['retrodicted masses']}
+
+2024-07-16 04:21:55,094 - INFO - Predicted Response:
+assistant
+
+property: accuracy
+
+2024-07-16 04:21:55,094 - INFO - Predicted Tag:
+{'property': ['accuracy']}
+
+2024-07-16 04:21:56,967 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Finally, the new atomic scale gravitational coupling constant suggests a radical revision of the assumptions governing the Planck scale, and leads to a natural explanation for the fine structure constant.
+Extractions:
+
+
+2024-07-16 04:21:56,968 - INFO - True Tag:
+{'object': ['gravitational coupling constant', 'Planck scale', 'fine structure constant']}
+
+2024-07-16 04:21:56,968 - INFO - Predicted Response:
+assistant
+
+property: fine structure constant
+
+2024-07-16 04:21:56,968 - INFO - Predicted Tag:
+{'property': ['fine structure constant']}
+
+2024-07-16 04:21:56,981 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746
+2024-07-16 04:21:56,982 - INFO - ##################################################
+2024-07-16 04:21:59,275 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Large-Scale Magnetic-Field Generation by Randomly Forced Shearing Waves
+Extractions:
+
+
+2024-07-16 04:21:59,275 - INFO - True Tag:
+{'task': ['Large-Scale Magnetic-Field Generation'], 'method': ['Randomly Forced Shearing Waves']}
+
+2024-07-16 04:21:59,275 - INFO - Predicted Response:
+assistant
+
+model: Large-Scale Magnetic-Field Generation
+
+2024-07-16 04:21:59,275 - INFO - Predicted Tag:
+{'model': ['Large-Scale Magnetic-Field Generation']}
+
+2024-07-16 04:22:04,293 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: A rigorous theory for the generation of a large-scale magnetic field by random non-helically forced motions of a conducting fluid combined with a linear shear is presented in the analytically tractable limit of low Rm and weak shear
+Extractions:
+
+
+2024-07-16 04:22:04,293 - INFO - True Tag:
+{'task': ['generation of a large-scale magnetic field'], 'object': ['magnetic field', 'conducting fluid'], 'method': ['random non-helically forced motions', 'linear shear']}
+
+2024-07-16 04:22:04,293 - INFO - Predicted Response:
+assistant
+
+model: rigorous theory
+method: random non-helically forced motions
+property: large-scale, low Rm, weak shear
+object: magnetic field, conducting fluid
+
+2024-07-16 04:22:04,293 - INFO - Predicted Tag:
+{'model': ['rigorous theory'], 'method': ['random non-helically forced motions'], 'property': ['large-scale', 'low Rm', 'weak shear'], 'object': ['magnetic field', 'conducting fluid']}
+
+2024-07-16 04:22:06,485 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The dynamo is kinematic and due to fluctuations in the net (volume-averaged) electromotive force
+Extractions:
+
+
+2024-07-16 04:22:06,486 - INFO - True Tag:
+{'property': ['dynamo', 'kinematic'], 'object': ['electromotive force']}
+
+2024-07-16 04:22:06,486 - INFO - Predicted Response:
+assistant
+
+object: dynamo, electromotive force
+
+2024-07-16 04:22:06,486 - INFO - Predicted Tag:
+{'object': ['dynamo', 'electromotive force']}
+
+2024-07-16 04:22:08,897 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: This is a minimal proof-of-concept quasilinear calculation aiming to put the shear dynamo, a new effect recently found in numerical experiments, on a firm theoretical footing
+Extractions:
+
+
+2024-07-16 04:22:08,898 - INFO - True Tag:
+{'property': ['shear dynamo']}
+
+2024-07-16 04:22:08,898 - INFO - Predicted Response:
+assistant
+
+model: quasilinear calculation, shear dynamo
+
+2024-07-16 04:22:08,898 - INFO - Predicted Tag:
+{'model': ['quasilinear calculation', 'shear dynamo']}
+
+2024-07-16 04:22:10,767 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Numerically observed scalings of the wavenumber and growth rate of the fastest growing mode, previously not understood, are derived analytically
+Extractions:
+
+
+2024-07-16 04:22:10,767 - INFO - True Tag:
+{'property': ['wavenumber', 'growth rate'], 'object': ['mode']}
+
+2024-07-16 04:22:10,767 - INFO - Predicted Response:
+assistant
+
+method: analytically
+
+2024-07-16 04:22:10,767 - INFO - Predicted Tag:
+{'method': ['analytically']}
+
+2024-07-16 04:22:12,746 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The simplicity of the model suggests that shear dynamo action may be a generic property of sheared magnetohydrodynamic turbulence.
+Extractions:
+
+
+2024-07-16 04:22:12,746 - INFO - True Tag:
+{'property': ['shear dynamo action'], 'object': ['magnetohydrodynamic turbulence']}
+
+2024-07-16 04:22:12,746 - INFO - Predicted Response:
+assistant
+
+model: shear dynamo action
+
+2024-07-16 04:22:12,747 - INFO - Predicted Tag:
+{'model': ['shear dynamo action']}
+
+2024-07-16 04:22:12,747 - INFO - ##################################################
+2024-07-16 04:22:15,482 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Sunyaev-Zel'dovich Effect Observations of the Bullet Cluster (1E 0657-56) with APEX-SZ
+Extractions:
+
+
+2024-07-16 04:22:15,482 - INFO - True Tag:
+{'object': ["Sunyaev-Zel'dovich Effect", 'Bullet Cluster (1E 0657-56)'], 'instrument': ['APEX-SZ']}
+
+2024-07-16 04:22:15,482 - INFO - Predicted Response:
+assistant
+
+object: Bullet Cluster, Sunyaev-Zel'dovich Effect
+
+2024-07-16 04:22:15,482 - INFO - Predicted Tag:
+{'object': ['Bullet Cluster', "Sunyaev-Zel'dovich Effect"]}
+
+2024-07-16 04:22:19,425 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We present observations of the Sunyaev-Zel'dovich effect (SZE) in the Bullet cluster (1E 0657--56) using the APEX-SZ instrument at 150 GHz with a resolution of 1 arcmin
+Extractions:
+
+
+2024-07-16 04:22:19,425 - INFO - True Tag:
+{'object': ["Sunyaev-Zel'dovich effect (SZE)", 'Bullet cluster (1E 0657--56)'], 'instrument': ['APEX-SZ']}
+
+2024-07-16 04:22:19,425 - INFO - Predicted Response:
+assistant
+
+instrument: APEX-SZ
+object: Sunyaev-Zel'dovich effect (SZE), Bullet cluster
+
+2024-07-16 04:22:19,425 - INFO - Predicted Tag:
+{'instrument': ['APEX-SZ'], 'object': ["Sunyaev-Zel'dovich effect (SZE)", 'Bullet cluster']}
+
+2024-07-16 04:22:21,505 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The main results are maps of the SZE in this massive, merging galaxy cluster
+Extractions:
+
+
+2024-07-16 04:22:21,505 - INFO - True Tag:
+{'object': ['SZE', 'galaxy cluster']}
+
+2024-07-16 04:22:21,505 - INFO - Predicted Response:
+assistant
+
+object: SZE, galaxy cluster
+
+2024-07-16 04:22:21,505 - INFO - Predicted Tag:
+{'object': ['SZE', 'galaxy cluster']}
+
+2024-07-16 04:22:23,155 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The cluster is detected with 23 sigma significance within the central 1 arcmin radius of the source position
+Extractions:
+
+
+2024-07-16 04:22:23,155 - INFO - True Tag:
+{'object': ['cluster'], 'property': ['radius']}
+
+2024-07-16 04:22:23,155 - INFO - Predicted Response:
+assistant
+
+property: significance
+
+2024-07-16 04:22:23,155 - INFO - Predicted Tag:
+{'property': ['significance']}
+
+2024-07-16 04:22:26,546 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The SZE map has a broadly similar morphology to that in existing X-ray maps of this system, and we find no evidence for significant contamination of the SZE emission by radio or IR sources
+Extractions:
+
+
+2024-07-16 04:22:26,546 - INFO - True Tag:
+{'object': ['SZE map', 'X-ray maps', 'SZE emission'], 'modality': ['X-ray', 'radio', 'IR']}
+
+2024-07-16 04:22:26,546 - INFO - Predicted Response:
+assistant
+
+object: SZE map, X-ray maps, SZE emission, radio sources, IR sources
+
+2024-07-16 04:22:26,546 - INFO - Predicted Tag:
+{'object': ['SZE map', 'X-ray maps', 'SZE emission', 'radio sources', 'IR sources']}
+
+2024-07-16 04:22:28,753 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In order to make simple quantitative comparisons with cluster gas models derived from X-ray observations, we fit our data to an isothermal elliptical beta model, despite the inadequacy of such a model for this complex merging system
+Extractions:
+
+
+2024-07-16 04:22:28,753 - INFO - True Tag:
+{'model': ['cluster gas models'], 'object': ['cluster gas'], 'dataset': ['X-ray observations'], 'modality': ['X-ray'], 'method': ['isothermal elliptical beta model']}
+
+2024-07-16 04:22:28,753 - INFO - Predicted Response:
+assistant
+
+model: isothermal elliptical beta model
+
+2024-07-16 04:22:28,753 - INFO - Predicted Tag:
+{'model': ['isothermal elliptical beta model']}
+
+2024-07-16 04:22:32,388 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: With an X-ray derived prior on the power-law index, beta = 1.04 +0.16 -0.10, we find a core radius r_c =142 +/- 18 arcsec, an axial ratio of 0.889 +/- 0.072, and a central temperature decrement of -771 +/- 71 micro-K_CMB, including a +/-5.5% flux calibration uncertainty
+Extractions:
+
+
+2024-07-16 04:22:32,389 - INFO - True Tag:
+{'modality': ['X-ray'], 'object': ['power-law index'], 'property': ['radius', 'axial ratio', 'temperature decrement', 'flux calibration uncertainty']}
+
+2024-07-16 04:22:32,389 - INFO - Predicted Response:
+assistant
+
+property: power-law index, beta, core radius, axial ratio, central temperature decrement, flux calibration uncertainty
+
+2024-07-16 04:22:32,389 - INFO - Predicted Tag:
+{'property': ['power-law index', 'beta', 'core radius', 'axial ratio', 'central temperature decrement', 'flux calibration uncertainty']}
+
+2024-07-16 04:22:37,853 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Combining the APEX-SZ map with a map of projected electron surface density from Chandra X-ray observations, we determine the mass-weighted temperature of the cluster gas to be T_mg=10.8 +/- 0.9 keV, significantly lower than some previously reported X-ray spectroscopic temperatures
+Extractions:
+
+
+2024-07-16 04:22:37,853 - INFO - True Tag:
+{'object': ['APEX-SZ map', 'cluster gas'], 'instrument': ['APEX-SZ', 'Chandra X-ray observations', 'X-ray observations'], 'dataset': ['Chandra X-ray observations'], 'modality': ['X-ray', 'X-ray spectroscopic'], 'property': ['mass-weighted', 'temperature']}
+
+2024-07-16 04:22:37,853 - INFO - Predicted Response:
+assistant
+
+dataset: APEX-SZ map, Chandra X-ray observations
+instrument: APEX-SZ, Chandra
+property: mass-weighted temperature, X-ray spectroscopic temperatures
+
+2024-07-16 04:22:37,853 - INFO - Predicted Tag:
+{'dataset': ['APEX-SZ map', 'Chandra X-ray observations'], 'instrument': ['APEX-SZ', 'Chandra'], 'property': ['mass-weighted temperature', 'X-ray spectroscopic temperatures']}
+
+2024-07-16 04:22:40,927 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Under the assumption of an isothermal cluster gas distribution in hydrostatic equilibrium, we compute the gas mass fraction for prolate and oblate spheroidal geometries and find it to be consistent with previous results from X-ray and weak lensing observations
+Extractions:
+
+
+2024-07-16 04:22:40,927 - INFO - True Tag:
+{'object': ['cluster gas', 'prolate', 'oblate spheroidal geometries'], 'property': ['gas mass fraction'], 'modality': ['X-ray', 'weak lensing']}
+
+2024-07-16 04:22:40,928 - INFO - Predicted Response:
+assistant
+
+model: isothermal cluster gas distribution
+object: gas, cluster, X-ray
+
+2024-07-16 04:22:40,928 - INFO - Predicted Tag:
+{'model': ['isothermal cluster gas distribution'], 'object': ['gas', 'cluster', 'X-ray']}
+
+2024-07-16 04:22:43,128 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: This work is the first result from the APEX-SZ experiment, and represents the first reported scientific result from observations with a large array of multiplexed superconducting transition-edge sensor bolometers.
+Extractions:
+
+
+2024-07-16 04:22:43,128 - INFO - True Tag:
+{'instrument': ['APEX-SZ', 'multiplexed superconducting transition-edge sensor bolometers']}
+
+2024-07-16 04:22:43,128 - INFO - Predicted Response:
+assistant
+
+instrument: APEX-SZ experiment
+
+2024-07-16 04:22:43,128 - INFO - Predicted Tag:
+{'instrument': ['APEX-SZ experiment']}
+
+2024-07-16 04:22:43,128 - INFO - ##################################################
+2024-07-16 04:22:45,092 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Natural Coordinate System in Curved Space-time
+Extractions:
+
+
+2024-07-16 04:22:45,092 - INFO - True Tag:
+{'model': ['Natural Coordinate System'], 'object': ['Curved Space-time']}
+
+2024-07-16 04:22:45,092 - INFO - Predicted Response:
+assistant
+
+field: Curved Space-time
+
+2024-07-16 04:22:45,092 - INFO - Predicted Tag:
+{'field': ['Curved Space-time']}
+
+2024-07-16 04:22:46,855 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In this paper we establish a generally and globally valid coordinate system in curved space-time with the simultaneous hypersurface orthogonal to the time coordinate
+Extractions:
+
+
+2024-07-16 04:22:46,855 - INFO - True Tag:
+{'model': ['coordinate system'], 'object': ['curved space-time', 'hypersurface orthogonal', 'time coordinate']}
+
+2024-07-16 04:22:46,855 - INFO - Predicted Response:
+assistant
+
+field: space-time
+
+2024-07-16 04:22:46,856 - INFO - Predicted Tag:
+{'field': ['space-time']}
+
+2024-07-16 04:22:48,936 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The time coordinate can be preseted according to practical evolving process and keep synchronous with the evolution of the realistic world
+Extractions:
+
+
+2024-07-16 04:22:48,936 - INFO - True Tag:
+{'object': ['time coordinate']}
+
+2024-07-16 04:22:48,936 - INFO - Predicted Response:
+assistant
+
+Extractions:
+property: time
+
+2024-07-16 04:22:48,936 - INFO - Predicted Tag:
+{'property': ['time']}
+
+2024-07-16 04:22:50,697 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In this coordinate system, it is convenient to express the physical laws and to calculate physical variables with clear geometrical meaning
+Extractions:
+
+
+2024-07-16 04:22:50,697 - INFO - True Tag:
+{'model': ['coordinate system'], 'property': ['geometrical']}
+
+2024-07-16 04:22:50,697 - INFO - Predicted Response:
+assistant
+
+Extractions:
+
+2024-07-16 04:22:50,697 - INFO - Predicted Tag:
+{}
+
+2024-07-16 04:22:52,438 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We call it "natural coordinate system"
+Extractions:
+
+
+2024-07-16 04:22:52,438 - INFO - True Tag:
+{'model': ['\\"natural coordinate system\\"']}
+
+2024-07-16 04:22:52,438 - INFO - Predicted Response:
+assistant
+
+No extractions.
+
+2024-07-16 04:22:52,439 - INFO - Predicted Tag:
+{}
+
+2024-07-16 04:22:54,199 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The constructing method for the natural coordinate system is concretely provided, and its physical and geometrical meanings are discussed in detail
+Extractions:
+
+
+2024-07-16 04:22:54,199 - INFO - True Tag:
+{'model': ['natural coordinate system'], 'property': ['physcial', 'geometrical']}
+
+2024-07-16 04:22:54,199 - INFO - Predicted Response:
+assistant
+
+method: constructing method
+
+2024-07-16 04:22:54,200 - INFO - Predicted Tag:
+{'method': ['constructing method']}
+
+2024-07-16 04:22:58,238 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In NCS we make classical approximation of spinor equation to get Newtonian mechanics, and then make weak field approximation of Einstein's equation and low speed approximation of particles moving in the space-time
+Extractions:
+
+
+2024-07-16 04:22:58,238 - INFO - True Tag:
+{'model': ['NCS'], 'method': ['classical approximation of spinor equation', "weak field approximation of Einstein's equation", 'low speed approximation of particles'], 'object': ['Newtonian mechanics', 'space-time']}
+
+2024-07-16 04:22:58,238 - INFO - Predicted Response:
+assistant
+
+model: classical approximation of spinor equation, Einstein's equation
+method: classical approximation, weak field approximation, low speed approximation
+
+2024-07-16 04:22:58,238 - INFO - Predicted Tag:
+{'model': ['classical approximation of spinor equation', "Einstein's equation"], 'method': ['classical approximation', 'weak field approximation', 'low speed approximation']}
+
+2024-07-16 04:23:00,004 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: From the analysis and examples we find it is a nice coordinate system to describe the realistic curved space-time, and is helpful to understand the nature of space-time.
+Extractions:
+
+
+2024-07-16 04:23:00,004 - INFO - True Tag:
+{'model': ['coordinate system'], 'object': ['curved space-time', 'space-time']}
+
+2024-07-16 04:23:00,004 - INFO - Predicted Response:
+assistant
+
+model: coordinate system
+
+2024-07-16 04:23:00,004 - INFO - Predicted Tag:
+{'model': ['coordinate system']}
+
+2024-07-16 04:23:00,020 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746
+2024-07-16 04:23:00,021 - INFO - ##################################################
+2024-07-16 04:23:01,552 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: 2MTF I
+Extractions:
+
+
+2024-07-16 04:23:01,552 - INFO - True Tag:
+{}
+
+2024-07-16 04:23:01,552 - INFO - Predicted Response:
+assistant
+
+field:
+
+2024-07-16 04:23:01,552 - INFO - Predicted Tag:
+{}
+
+2024-07-16 04:23:03,634 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The Tully-Fisher Relation in the 2MASS J, H and K Bands
+Extractions:
+
+
+2024-07-16 04:23:03,634 - INFO - True Tag:
+{'method': ['The Tully-Fisher Relation'], 'object': ['the 2MASS J, H and K Bands']}
+
+2024-07-16 04:23:03,634 - INFO - Predicted Response:
+assistant
+
+object: Tully-Fisher Relation
+
+2024-07-16 04:23:03,634 - INFO - Predicted Tag:
+{'object': ['Tully-Fisher Relation']}
+
+2024-07-16 04:23:10,610 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The 2 Micron All-Sky Survey (2MASS) Tully-Fisher Survey (2MTF) aims to measure Tully-Fisher (TF) distances to all bright inclined spirals in the 2MASS Redshift Survey (2MRS)
+Extractions:
+
+
+2024-07-16 04:23:10,610 - INFO - True Tag:
+{'dataset': ['The 2 Micron All-Sky Survey (2MASS)', 'Tully-Fisher Survey (2MTF)', 'the 2MASS Redshift Survey (2MRS)'], 'property': ['Tully-Fisher (TF) distances'], 'object': ['bright inclined spirals']}
+
+2024-07-16 04:23:10,610 - INFO - Predicted Response:
+assistant
+
+dataset: 2 Micron All-Sky Survey (2MASS), 2MASS Redshift Survey (2MRS)
+instrument: 2 Micron All-Sky Survey (2MASS)
+object: Tully-Fisher distances, spirals
+
+2024-07-16 04:23:10,610 - INFO - Predicted Tag:
+{'dataset': ['2 Micron All-Sky Survey (2MASS)', '2MASS Redshift Survey (2MRS)'], 'instrument': ['2 Micron All-Sky Survey (2MASS)'], 'object': ['Tully-Fisher distances', 'spirals']}
+
+2024-07-16 04:23:12,383 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Essential to this project is a universal calibration of the TF relation in the 2MASS J (1.2 um), H (1.6 um) and K (2.2 um) bands
+Extractions:
+
+
+2024-07-16 04:23:12,383 - INFO - True Tag:
+{'method': ['universal calibration', 'TF relation'], 'object': ['the 2MASS J (1.2 um), H (1.6 um) and K (2.2 um) bands']}
+
+2024-07-16 04:23:12,383 - INFO - Predicted Response:
+assistant
+
+method: TF relation
+
+2024-07-16 04:23:12,383 - INFO - Predicted Tag:
+{'method': ['TF relation']}
+
+2024-07-16 04:23:14,135 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We present the first bias corrected or universal TF template in these bands
+Extractions:
+
+
+2024-07-16 04:23:14,135 - INFO - True Tag:
+{'model': ['bias corrected or universal TF template']}
+
+2024-07-16 04:23:14,135 - INFO - Predicted Response:
+assistant
+
+model: TF template
+
+2024-07-16 04:23:14,136 - INFO - Predicted Tag:
+{'model': ['TF template']}
+
+2024-07-16 04:23:17,528 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We find that the slope of the TF relation becomes steeper as the wavelength increases being close to L \propto v^4 in K-band and L \propto v^3.6 in J and H-bands
+Extractions:
+
+
+2024-07-16 04:23:17,528 - INFO - True Tag:
+{'method': ['TF relation'], 'property': ['the wavelength'], 'object': ['K-band', 'J and H-bands']}
+
+2024-07-16 04:23:17,528 - INFO - Predicted Response:
+assistant
+
+property: slope, wavelength
+object: TF relation, K-band, J, H-bands
+
+2024-07-16 04:23:17,528 - INFO - Predicted Tag:
+{'property': ['slope', 'wavelength'], 'object': ['TF relation', 'K-band', 'J', 'H-bands']}
+
+2024-07-16 04:23:19,947 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We also investigate the dependence on galaxy morphology showing that in all three bands the relation is steeper for later type spirals which also have a dimmer TF zeropoint than earlier type spirals
+Extractions:
+
+
+2024-07-16 04:23:19,947 - INFO - True Tag:
+{'property': ['galaxy morphology', 'TF zeropoint'], 'object': ['later type spirals', 'earlier type spirals']}
+
+2024-07-16 04:23:19,947 - INFO - Predicted Response:
+assistant
+
+object: galaxy, spirals
+property: morphology
+
+2024-07-16 04:23:19,947 - INFO - Predicted Tag:
+{'object': ['galaxy', 'spirals'], 'property': ['morphology']}
+
+2024-07-16 04:23:21,701 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We correct the final relation to that for Sc galaxies
+Extractions:
+
+
+2024-07-16 04:23:21,701 - INFO - True Tag:
+{'object': ['Sc galaxies']}
+
+2024-07-16 04:23:21,701 - INFO - Predicted Response:
+assistant
+
+field: Sc galaxies
+
+2024-07-16 04:23:21,701 - INFO - Predicted Tag:
+{'field': ['Sc galaxies']}
+
+2024-07-16 04:23:23,679 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Finally we study the scatter from the TF relation fitting for a width dependent intrinsic scatter which is not found to vary significantly with wavelength.
+Extractions:
+
+
+2024-07-16 04:23:23,679 - INFO - True Tag:
+{'method': ['TF relation'], 'object': ['wavelength']}
+
+2024-07-16 04:23:23,679 - INFO - Predicted Response:
+assistant
+
+property: width, intrinsic scatter
+
+2024-07-16 04:23:23,679 - INFO - Predicted Tag:
+{'property': ['width', 'intrinsic scatter']}
+
+2024-07-16 04:23:23,679 - INFO - ##################################################
+2024-07-16 04:23:26,734 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The S1 Shell and Interstellar Magnetic Field and Gas near the Heliosphere
+Extractions:
+
+
+2024-07-16 04:23:26,734 - INFO - True Tag:
+{'object': ['S1 Shell', 'Interstellar Magnetic Field', 'the Heliosphere']}
+
+2024-07-16 04:23:26,734 - INFO - Predicted Response:
+assistant
+
+object: S1 Shell, Interstellar Magnetic Field, Gas, Heliosphere
+
+2024-07-16 04:23:26,734 - INFO - Predicted Tag:
+{'object': ['S1 Shell', 'Interstellar Magnetic Field', 'Gas', 'Heliosphere']}
+
+2024-07-16 04:23:29,035 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Many studies of the Loop I magnetic superbubble place the Sun at the edges of the bubble
+Extractions:
+
+
+2024-07-16 04:23:29,035 - INFO - True Tag:
+{'object': ['Loop I magnetic superbubble', 'the Sun']}
+
+2024-07-16 04:23:29,035 - INFO - Predicted Response:
+assistant
+
+object: Loop I magnetic superbubble, Sun
+
+2024-07-16 04:23:29,035 - INFO - Predicted Tag:
+{'object': ['Loop I magnetic superbubble', 'Sun']}
+
+2024-07-16 04:23:32,205 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: One recent study models the polarized radio continuum of Loop I as two magnetic shells with the Sun embedded in the rim of the 'S1' shell
+Extractions:
+
+
+2024-07-16 04:23:32,205 - INFO - True Tag:
+{'object': ['the polarized radio continuum', 'Loop I', 'magnetic shells', 'the Sun', "the 'S1' shell"]}
+
+2024-07-16 04:23:32,205 - INFO - Predicted Response:
+assistant
+
+model: magnetic shells
+object: Loop I, Sun, 'S1' shell
+
+2024-07-16 04:23:32,205 - INFO - Predicted Tag:
+{'model': ['magnetic shells'], 'object': ['Loop I', 'Sun', "'S1' shell"]}
+
+2024-07-16 04:23:34,835 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: If the Sun is in such a shell, it should be apparent in both the local interstellar magnetic field and the distribution of nearby interstellar material
+Extractions:
+
+
+2024-07-16 04:23:34,835 - INFO - True Tag:
+{'object': ['the Sun', 'the local interstellar magnetic field', 'interstellar material']}
+
+2024-07-16 04:23:34,835 - INFO - Predicted Response:
+assistant
+
+object: Sun, interstellar magnetic field, interstellar material
+
+2024-07-16 04:23:34,835 - INFO - Predicted Tag:
+{'object': ['Sun', 'interstellar magnetic field', 'interstellar material']}
+
+2024-07-16 04:23:39,095 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The properties of these subshells are compared to optical polarization data that trace the nearby interstellar magnetic field (ISMF), and the distribution of interstellar FeII and CaII within about 55 pc of the Sun
+Extractions:
+
+
+2024-07-16 04:23:39,095 - INFO - True Tag:
+{'modality': ['optical polarization data'], 'object': ['interstellar magnetic field (ISMF)', 'interstellar FeII and CaII', 'the Sun']}
+
+2024-07-16 04:23:39,096 - INFO - Predicted Response:
+assistant
+
+object: subshells, interstellar magnetic field (ISMF), interstellar FeII, CaII, Sun
+property: properties
+
+2024-07-16 04:23:39,096 - INFO - Predicted Tag:
+{'object': ['subshells', 'interstellar magnetic field (ISMF)', 'interstellar FeII', 'CaII', 'Sun'], 'property': ['properties']}
+
+2024-07-16 04:23:41,403 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The result is that a model of Loop I as composed of two magnetic subshells is a viable description of the distribution of nearby low density ISM
+Extractions:
+
+
+2024-07-16 04:23:41,403 - INFO - True Tag:
+{'object': ['Loop I', 'magnetic subshells', 'low density ISM']}
+
+2024-07-16 04:23:41,403 - INFO - Predicted Response:
+assistant
+
+model: Loop I
+object: ISM
+
+2024-07-16 04:23:41,403 - INFO - Predicted Tag:
+{'model': ['Loop I'], 'object': ['ISM']}
+
+2024-07-16 04:23:45,229 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Column densities of the recombinant ion CaII are found to increase with the strength of the interstellar radiation field, rather than with star distance or total pathlength through the two magnetic subshells
+Extractions:
+
+
+2024-07-16 04:23:45,229 - INFO - True Tag:
+{'property': ['Column densities', 'star distance', 'total pathlength'], 'object': ['the recombinant ion CaII', 'the interstellar radiation field', 'magnetic subshells']}
+
+2024-07-16 04:23:45,229 - INFO - Predicted Response:
+assistant
+
+object: CaII, interstellar radiation field, star, magnetic subshells
+property: column densities, strength
+
+2024-07-16 04:23:45,229 - INFO - Predicted Tag:
+{'object': ['CaII', 'interstellar radiation field', 'star', 'magnetic subshells'], 'property': ['column densities', 'strength']}
+
+2024-07-16 04:23:48,402 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: As found earlier, the symmetry of the dipole moment of the cosmic microwave background corresponds to the symmetries of the heliosphere and local ISMF (to within 10 degrees).
+Extractions:
+
+
+2024-07-16 04:23:48,402 - INFO - True Tag:
+{'property': ['the dipole moment'], 'object': ['the cosmic microwave background', 'the heliosphere', 'local ISMF']}
+
+2024-07-16 04:23:48,402 - INFO - Predicted Response:
+assistant
+
+object: dipole moment, cosmic microwave background, heliosphere, local ISMF
+
+2024-07-16 04:23:48,402 - INFO - Predicted Tag:
+{'object': ['dipole moment', 'cosmic microwave background', 'heliosphere', 'local ISMF']}
+
+2024-07-16 04:23:48,402 - INFO - ##################################################
+2024-07-16 04:23:51,891 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The growth of supermassive black holes in pseudo-bulges, classical bulges and elliptical galaxies
+Extractions:
+
+
+2024-07-16 04:23:51,891 - INFO - True Tag:
+{'object': ['supermassive black holes', 'pseudo-bulges', 'classical bulges', 'elliptical galaxies']}
+
+2024-07-16 04:23:51,891 - INFO - Predicted Response:
+assistant
+
+object: supermassive black holes, pseudo-bulges, classical bulges, elliptical galaxies
+
+2024-07-16 04:23:51,891 - INFO - Predicted Tag:
+{'object': ['supermassive black holes', 'pseudo-bulges', 'classical bulges', 'elliptical galaxies']}
+
+2024-07-16 04:23:57,353 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Using results from structural analysis of a sample of nearly 1000 local galaxies from the Sloan Digital Sky Survey, we estimate how the mass in central black holes is distributed amongst elliptical galaxies, classical bulges and pseudo-bulges, and investigate the relation between their stellar masses and central stellar velocity dispersion sigma
+Extractions:
+
+
+2024-07-16 04:23:57,353 - INFO - True Tag:
+{'method': ['structural analysis'], 'object': ['local galaxies', 'central black holes', 'elliptical galaxies', 'classical bulges', 'pseudo-bulges'], 'dataset': ['Sloan Digital Sky Survey'], 'property': ['mass', 'stellar masses', 'central stellar velocity dispersion sigma']}
+
+2024-07-16 04:23:57,353 - INFO - Predicted Response:
+assistant
+
+dataset: Sloan Digital Sky Survey
+object: galaxies, elliptical galaxies, classical bulges, pseudo-bulges, black holes
+property: mass, stellar masses, central stellar velocity dispersion
+
+2024-07-16 04:23:57,353 - INFO - Predicted Tag:
+{'dataset': ['Sloan Digital Sky Survey'], 'object': ['galaxies', 'elliptical galaxies', 'classical bulges', 'pseudo-bulges', 'black holes'], 'property': ['mass', 'stellar masses', 'central stellar velocity dispersion']}
+
+2024-07-16 04:24:01,650 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Assuming a single relation between elliptical galaxy/bulge mass, M_Bulge, and central black hole mass, M_BH, we find that 55^{+8}_{-4} per cent of the mass in black holes in the local universe is in the centres of elliptical galaxies, 41^{+4}_{-2} per cent in classical bulges and 4^{+0.9}_{-0.4} per cent in pseudo-bulges
+Extractions:
+
+
+2024-07-16 04:24:01,650 - INFO - True Tag:
+{'property': ['elliptical galaxy/bulge mass', 'central black hole mass', 'mass'], 'object': ['black holes', 'local universe', 'elliptical galaxies', 'classical bulges', 'pseudo-bulges']}
+
+2024-07-16 04:24:01,650 - INFO - Predicted Response:
+assistant
+
+object: elliptical galaxy, bulge, black hole, local universe, classical bulges, pseudo-bulges
+property: mass
+
+2024-07-16 04:24:01,650 - INFO - Predicted Tag:
+{'object': ['elliptical galaxy', 'bulge', 'black hole', 'local universe', 'classical bulges', 'pseudo-bulges'], 'property': ['mass']}
+
+2024-07-16 04:24:05,256 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We find that ellipticals, classical bulges and pseudo-bulges follow different relations between their stellar masses and sigma, and the most significant offset occurs for pseudo-bulges in barred galaxies
+Extractions:
+
+
+2024-07-16 04:24:05,256 - INFO - True Tag:
+{'object': ['ellipticals', 'classical bulges', 'pseudo-bulges', 'barred galaxies'], 'property': ['stellar masses', 'sigma']}
+
+2024-07-16 04:24:05,256 - INFO - Predicted Response:
+assistant
+
+object: ellipticals, classical bulges, pseudo-bulges, stellar masses, sigma, barred galaxies
+
+2024-07-16 04:24:05,256 - INFO - Predicted Tag:
+{'object': ['ellipticals', 'classical bulges', 'pseudo-bulges', 'stellar masses', 'sigma', 'barred galaxies']}
+
+2024-07-16 04:24:08,643 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: This structural dissimilarity leads to discrepant black hole masses if single M_BH-M_Bulge and M_BH-sigma relations are used
+Extractions:
+
+
+2024-07-16 04:24:08,643 - INFO - True Tag:
+{'property': ['black hole masses']}
+
+2024-07-16 04:24:08,643 - INFO - Predicted Response:
+assistant
+
+object: black hole, M_BH-M_Bulge, M_BH-sigma relations
+
+2024-07-16 04:24:08,643 - INFO - Predicted Tag:
+{'object': ['black hole', 'M_BH-M_Bulge', 'M_BH-sigma relations']}
+
+2024-07-16 04:24:10,527 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Adopting relations from the literature, we find that the M_BH-sigma relation yields an estimate of the total mass density in black holes that is roughly 55 per cent larger than if the M_BH-M_Bulge relation is used.
+Extractions:
+
+
+2024-07-16 04:24:10,527 - INFO - True Tag:
+{'property': ['total mass density'], 'object': ['black holes']}
+
+2024-07-16 04:24:10,528 - INFO - Predicted Response:
+assistant
+
+property: total mass density
+
+2024-07-16 04:24:10,528 - INFO - Predicted Tag:
+{'property': ['total mass density']}
+
+2024-07-16 04:24:10,544 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746
+2024-07-16 04:24:10,544 - INFO - ##################################################
+2024-07-16 04:24:13,161 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Characteristic Scales of Initial Density and Velocity Fields
+Extractions:
+
+
+2024-07-16 04:24:13,161 - INFO - True Tag:
+{'property': ['Characteristic Scales'], 'object': ['Initial Density and Velocity Fields']}
+
+2024-07-16 04:24:13,161 - INFO - Predicted Response:
+assistant
+
+property: Characteristic Scales, Initial Density, Velocity Fields
+
+2024-07-16 04:24:13,161 - INFO - Predicted Tag:
+{'property': ['Characteristic Scales', 'Initial Density', 'Velocity Fields']}
+
+2024-07-16 04:24:16,553 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: For the initial fields of the density contrast and peculiar velocity, we theoretically calculate the differential and integral length scales, i.e., statistical measures that respectively characterize the small- and large-scale fluctuations of a random field
+Extractions:
+
+
+2024-07-16 04:24:16,553 - INFO - True Tag:
+{'object': ['initial fields', 'density contrast', 'peculiar velocity', 'random field'], 'property': ['differential and integral length scales']}
+
+2024-07-16 04:24:16,553 - INFO - Predicted Response:
+assistant
+
+property: density contrast, peculiar velocity, differential length scales, integral length scales
+object: field
+
+2024-07-16 04:24:16,553 - INFO - Predicted Tag:
+{'property': ['density contrast', 'peculiar velocity', 'differential length scales', 'integral length scales'], 'object': ['field']}
+
+2024-07-16 04:24:18,874 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: These length scales and the associated mass scales explain the length and mass scales observed for (1) halos of young galaxies at z > 5, (2) halos of galaxies at z = 0, and (3) the largest structures in the galaxy distribution at z = 0
+Extractions:
+
+
+2024-07-16 04:24:18,874 - INFO - True Tag:
+{'property': ['length scales', 'mass scales', 'length and mass scales'], 'object': ['halos of young galaxies', 'halos of galaxies', 'galaxy distribution']}
+
+2024-07-16 04:24:18,874 - INFO - Predicted Response:
+assistant
+
+object: halos, galaxies, galaxy distribution
+
+2024-07-16 04:24:18,874 - INFO - Predicted Tag:
+{'object': ['halos', 'galaxies', 'galaxy distribution']}
+
+2024-07-16 04:24:20,740 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We thereby discuss that such observed scales are fossil imprints of the characteristic scales of the initial fields.
+Extractions:
+
+
+2024-07-16 04:24:20,740 - INFO - True Tag:
+{'property': ['characteristic scales', 'initial fields']}
+
+2024-07-16 04:24:20,740 - INFO - Predicted Response:
+assistant
+
+object: scales, fields
+
+2024-07-16 04:24:20,740 - INFO - Predicted Tag:
+{'object': ['scales', 'fields']}
+
+2024-07-16 04:24:20,741 - INFO - ##################################################
+2024-07-16 04:24:23,791 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Gravitino Dark Matter and the Flavour Structure of R-violating Operators
+Extractions:
+
+
+2024-07-16 04:24:23,791 - INFO - True Tag:
+{'object': ['Gravitino Dark Matter', 'R-violating Operators']}
+
+2024-07-16 04:24:23,791 - INFO - Predicted Response:
+assistant
+
+object: Gravitino Dark Matter, Flavour Structure, R-violating Operators
+
+2024-07-16 04:24:23,791 - INFO - Predicted Tag:
+{'object': ['Gravitino Dark Matter', 'Flavour Structure', 'R-violating Operators']}
+
+2024-07-16 04:24:27,290 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We study gravitino dark matter and slow gravitino decays within the framework of R-violating supersymmetry, with particular emphasis on the flavour dependence of the branching ratios and the allowed R-violating couplings
+Extractions:
+
+
+2024-07-16 04:24:27,290 - INFO - True Tag:
+{'object': ['gravitino dark matter', 'gravitino decays', 'R-violating supersymmetry', 'R-violating couplings'], 'property': ['flavour dependence']}
+
+2024-07-16 04:24:27,290 - INFO - Predicted Response:
+assistant
+
+model: R-violating supersymmetry
+object: gravitino dark matter, gravitino
+
+2024-07-16 04:24:27,290 - INFO - Predicted Tag:
+{'model': ['R-violating supersymmetry'], 'object': ['gravitino dark matter', 'gravitino']}
+
+2024-07-16 04:24:29,911 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The dominant decay modes and final state products turn out to be very sensitive to the R-violating hierarchies
+Extractions:
+
+
+2024-07-16 04:24:29,911 - INFO - True Tag:
+{'property': ['decay modes', 'final state products']}
+
+2024-07-16 04:24:29,911 - INFO - Predicted Response:
+assistant
+
+property: dominant decay modes, R-violating hierarchies
+
+2024-07-16 04:24:29,911 - INFO - Predicted Tag:
+{'property': ['dominant decay modes', 'R-violating hierarchies']}
+
+2024-07-16 04:24:32,106 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Mixing effects can be crucial in correctly deriving the relative magnitude of the various contributions, particularly for heavy flavours with phase space suppression
+Extractions:
+
+
+2024-07-16 04:24:32,106 - INFO - True Tag:
+{'method': ['Mixing effects'], 'property': ['magnitude', 'phase space suppression']}
+
+2024-07-16 04:24:32,106 - INFO - Predicted Response:
+assistant
+
+property: relative magnitude, phase space suppression
+
+2024-07-16 04:24:32,106 - INFO - Predicted Tag:
+{'property': ['relative magnitude', 'phase space suppression']}
+
+2024-07-16 04:24:35,720 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The study of the strength of different decay rates for the gravitino is also correlated to collider signatures expected from decays of the Next-to-Lightest Supersymmetric Particle (NLSP) and to single superparticle production.
+Extractions:
+
+
+2024-07-16 04:24:35,720 - INFO - True Tag:
+{'property': ['strength of different decay rates'], 'object': ['gravitino', 'Next-to-Lightest Supersymmetric Particle', 'superparticle']}
+
+2024-07-16 04:24:35,720 - INFO - Predicted Response:
+assistant
+
+object: gravitino, Next-to-Lightest Supersymmetric Particle (NLSP), superparticle
+
+2024-07-16 04:24:35,720 - INFO - Predicted Tag:
+{'object': ['gravitino', 'Next-to-Lightest Supersymmetric Particle (NLSP)', 'superparticle']}
+
+2024-07-16 04:24:35,721 - INFO - ##################################################
+2024-07-16 04:24:38,221 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Dark Matter Caustics in Galaxy Clusters
+Extractions:
+
+
+2024-07-16 04:24:38,221 - INFO - True Tag:
+{'object': ['Dark Matter Caustics', 'Galaxy Clusters']}
+
+2024-07-16 04:24:38,221 - INFO - Predicted Response:
+assistant
+
+object: Dark Matter Caustics, Galaxy Clusters
+
+2024-07-16 04:24:38,221 - INFO - Predicted Tag:
+{'object': ['Dark Matter Caustics', 'Galaxy Clusters']}
+
+2024-07-16 04:24:40,512 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We interpret the recent gravitational lensing observations of Jee et al
+Extractions:
+
+
+2024-07-16 04:24:40,512 - INFO - True Tag:
+{'modality': ['gravitational lensing observations'], 'object': ['gravitational lensing']}
+
+2024-07-16 04:24:40,512 - INFO - Predicted Response:
+assistant
+
+object: gravitational lensing observations, Jee
+
+2024-07-16 04:24:40,512 - INFO - Predicted Tag:
+{'object': ['gravitational lensing observations', 'Jee']}
+
+2024-07-16 04:24:43,136 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: \cite{Jee} as first evidence for a {\it caustic} ring of dark matter in a galaxy cluster
+Extractions:
+
+
+2024-07-16 04:24:43,136 - INFO - True Tag:
+{'object': ['{\\\\it caustic} ring', 'dark matter', 'galaxy cluster']}
+
+2024-07-16 04:24:43,136 - INFO - Predicted Response:
+assistant
+
+object: caustic ring, dark matter, galaxy cluster
+
+2024-07-16 04:24:43,137 - INFO - Predicted Tag:
+{'object': ['caustic ring', 'dark matter', 'galaxy cluster']}
+
+2024-07-16 04:24:45,005 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: A caustic ring unavoidably forms when a cold collisionless flow falls with net overall rotation in and out of a gravitational potential well
+Extractions:
+
+
+2024-07-16 04:24:45,005 - INFO - True Tag:
+{'object': ['caustic ring', 'flow', 'gravitational potential well'], 'property': ['cold', 'collisionless', 'net overall rotation']}
+
+2024-07-16 04:24:45,006 - INFO - Predicted Response:
+assistant
+
+model: gravitational potential well
+
+2024-07-16 04:24:45,006 - INFO - Predicted Tag:
+{'model': ['gravitational potential well']}
+
+2024-07-16 04:24:47,955 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Evidence for caustic rings of dark matter was previously found in the Milky Way and other isolated spiral galaxies
+Extractions:
+
+
+2024-07-16 04:24:47,955 - INFO - True Tag:
+{'object': ['caustic rings', 'dark matter', 'Milky Way', 'galaxies'], 'property': ['isolated', 'spiral']}
+
+2024-07-16 04:24:47,955 - INFO - Predicted Response:
+assistant
+
+object: caustic rings, dark matter, Milky Way, spiral galaxies
+
+2024-07-16 04:24:47,955 - INFO - Predicted Tag:
+{'object': ['caustic rings', 'dark matter', 'Milky Way', 'spiral galaxies']}
+
+2024-07-16 04:24:50,257 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We argue that galaxy clusters have at least one and possibly two or three caustic rings
+Extractions:
+
+
+2024-07-16 04:24:50,257 - INFO - True Tag:
+{'object': ['galaxy clusters', 'caustic rings']}
+
+2024-07-16 04:24:50,258 - INFO - Predicted Response:
+assistant
+
+object: galaxy clusters, caustic rings
+
+2024-07-16 04:24:50,258 - INFO - Predicted Tag:
+{'object': ['galaxy clusters', 'caustic rings']}
+
+2024-07-16 04:24:55,154 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: We calculate the column density profile of a caustic ring in a cluster and show that it is consistent with the observations of Jee et al.
+Extractions:
+
+
+2024-07-16 04:24:55,154 - INFO - True Tag:
+{'task': ['calculate the column density profile', 'show that it is consistent with the observations of'], 'property': ['column density profile'], 'object': ['caustic ring', 'cluster']}
+
+2024-07-16 04:24:55,154 - INFO - Predicted Response:
+assistant
+
+model: 
+task: 
+dataset: 
+field: 
+modality: 
+method: 
+object: caustic ring, cluster
+property: column density profile
+
+2024-07-16 04:24:55,154 - INFO - Predicted Tag:
+{'object': ['caustic ring', 'cluster'], 'property': ['column density profile']}
+
+2024-07-16 04:24:55,170 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746
+2024-07-16 04:24:55,171 - INFO - ##################################################
+2024-07-16 04:24:56,921 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Dark matter in elliptical galaxies: II
+Extractions:
+
+
+2024-07-16 04:24:56,921 - INFO - True Tag:
+{'object': ['Dark matter', 'elliptical galaxies']}
+
+2024-07-16 04:24:56,921 - INFO - Predicted Response:
+assistant
+
+field: dark matter
+
+2024-07-16 04:24:56,922 - INFO - Predicted Tag:
+{'field': ['dark matter']}
+
+2024-07-16 04:24:58,778 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Estimating the mass within the virial radius
+Extractions:
+
+
+2024-07-16 04:24:58,778 - INFO - True Tag:
+{'task': ['Estimating the mass within the virial radius'], 'property': ['mass', 'virial radius']}
+
+2024-07-16 04:24:58,778 - INFO - Predicted Response:
+assistant
+
+task: estimating the mass
+
+2024-07-16 04:24:58,778 - INFO - Predicted Tag:
+{'task': ['estimating the mass']}
+
+2024-07-16 04:25:02,929 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Elliptical galaxies are modelled with a a 4-component model: Sersic stars, LCDM dark matter (DM), hot gas and central black hole
+Extractions:
+
+
+2024-07-16 04:25:02,930 - INFO - True Tag:
+{'object': ['Elliptical galaxies', 'Sersic stars', 'dark matter', 'gas', 'black hole'], 'task': ['modelled'], 'model': ['4-component model', 'LCDM'], 'property': ['4-component', 'hot', 'central']}
+
+2024-07-16 04:25:02,930 - INFO - Predicted Response:
+assistant
+
+model: 4-component model
+object: elliptical galaxies, stars, dark matter (DM), hot gas, central black hole
+
+2024-07-16 04:25:02,930 - INFO - Predicted Tag:
+{'model': ['4-component model'], 'object': ['elliptical galaxies', 'stars', 'dark matter (DM)', 'hot gas', 'central black hole']}
+
+2024-07-16 04:25:05,225 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: DM is negligible in the inner regions, which are dominated by stars and the central black hole
+Extractions:
+
+
+2024-07-16 04:25:05,225 - INFO - True Tag:
+{'object': ['inner regions', 'stars', 'black hole'], 'property': ['central']}
+
+2024-07-16 04:25:05,226 - INFO - Predicted Response:
+assistant
+
+object: DM, stars, central black hole
+
+2024-07-16 04:25:05,226 - INFO - Predicted Tag:
+{'object': ['DM', 'stars', 'central black hole']}
+
+2024-07-16 04:25:07,096 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: This prevents any kinematical estimate (using a Jeans analysis) of the inner slope of the DM density profile
+Extractions:
+
+
+2024-07-16 04:25:07,096 - INFO - True Tag:
+{'method': ['Jeans analysis'], 'property': ['inner slope'], 'object': ['DM density profile']}
+
+2024-07-16 04:25:07,096 - INFO - Predicted Response:
+assistant
+
+model: DM density profile
+
+2024-07-16 04:25:07,096 - INFO - Predicted Tag:
+{'model': ['DM density profile']}
+
+2024-07-16 04:25:10,699 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The gas fraction rises, but the baryon fraction decreases with radius, at least out to 10 effective radii (R_e)
+Extractions:
+
+
+2024-07-16 04:25:10,699 - INFO - True Tag:
+{'property': ['gas fraction', 'baryon fraction', 'radius', 'effective radii']}
+
+2024-07-16 04:25:10,699 - INFO - Predicted Response:
+assistant
+
+property: gas fraction, baryon fraction
+object: radius, effective radii (R_e)
+
+2024-07-16 04:25:10,699 - INFO - Predicted Tag:
+{'property': ['gas fraction', 'baryon fraction'], 'object': ['radius', 'effective radii (R_e)']}
+
+2024-07-16 04:25:14,314 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Even with line-of-sight velocity dispersion (VD) measurements at 4 to 6 R_e with 20 km/s accuracy and perfectly known velocity anisotropy, the total mass within the virial radius (r_v) is uncertain by a factor over 3
+Extractions:
+
+
+2024-07-16 04:25:14,314 - INFO - True Tag:
+{'property': ['line-of-sight velocity dispersion', 'velocity anisotropy', 'mass', 'virial radius']}
+
+2024-07-16 04:25:14,314 - INFO - Predicted Response:
+assistant
+
+property: line-of-sight velocity dispersion, velocity anisotropy, total mass
+object: velocity
+
+2024-07-16 04:25:14,314 - INFO - Predicted Tag:
+{'property': ['line-of-sight velocity dispersion', 'velocity anisotropy', 'total mass'], 'object': ['velocity']}
+
+2024-07-16 04:25:17,592 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The DM distributions found in LCDM simulations are consistent with the stellar VD profiles, but appear inconsistent with the low VDs measured by Romanowsky et al
+Extractions:
+
+
+2024-07-16 04:25:17,592 - INFO - True Tag:
+{'method': ['LCDM simulations'], 'model': ['LCDM'], 'modality': ['stellar VD profiles']}
+
+2024-07-16 04:25:17,592 - INFO - Predicted Response:
+assistant
+
+model: LCDM simulations
+object: DM distributions, stellar VD profiles, VDs
+
+2024-07-16 04:25:17,592 - INFO - Predicted Tag:
+{'model': ['LCDM simulations'], 'object': ['DM distributions', 'stellar VD profiles', 'VDs']}
+
+2024-07-16 04:25:20,124 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: (2003) of planetary nebulae between 2 and 5 R_e, which imply such low M/Ls that the baryon fraction within r_v must be greater than the universal value
+Extractions:
+
+
+2024-07-16 04:25:20,124 - INFO - True Tag:
+{'object': ['planetary nebulae'], 'property': ['baryon fraction']}
+
+2024-07-16 04:25:20,124 - INFO - Predicted Response:
+assistant
+
+object: planetary nebulae, baryon fraction
+
+2024-07-16 04:25:20,124 - INFO - Predicted Tag:
+{'object': ['planetary nebulae', 'baryon fraction']}
+
+2024-07-16 04:25:22,635 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Replacing the NFW DM model by the new model of Navarro et al
+Extractions:
+
+
+2024-07-16 04:25:22,635 - INFO - True Tag:
+{'model': ['NFW DM model', 'model of Navarro et al']}
+
+2024-07-16 04:25:22,635 - INFO - Predicted Response:
+assistant
+
+model: NFW DM model, Navarro et al
+
+2024-07-16 04:25:22,635 - INFO - Predicted Tag:
+{'model': ['NFW DM model', 'Navarro et al']}
+
+2024-07-16 04:25:24,392 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: (2004) decreases slightly the VD at a given radius
+Extractions:
+
+
+2024-07-16 04:25:24,392 - INFO - True Tag:
+{'property': ['radius']}
+
+2024-07-16 04:25:24,392 - INFO - Predicted Response:
+assistant
+
+Extractions:
+
+2024-07-16 04:25:24,392 - INFO - Predicted Tag:
+{}
+
+2024-07-16 04:25:26,267 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: So, given the observed VD measured at 5 R_e, the inferred M/L within r_v is 40% larger than predicted with the NFW model
+Extractions:
+
+
+2024-07-16 04:25:26,267 - INFO - True Tag:
+{'model': ['NFW model']}
+
+2024-07-16 04:25:26,268 - INFO - Predicted Response:
+assistant
+
+model: NFW model
+
+2024-07-16 04:25:26,268 - INFO - Predicted Tag:
+{'model': ['NFW model']}
+
+2024-07-16 04:25:29,575 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Folding in the slight (strong) radial anisotropy found in LCDM (merger) simulations, which is well modelled (much better than with the Osipkov-Merritt formula) with beta(r) = 1/2 r/(r+a), the inferred M/L within r_v is another 1.6 (2.4) times higher than for the isotropic NFW model
+Extractions:
+
+
+2024-07-16 04:25:29,575 - INFO - True Tag:
+{'property': ['radial anisotropy'], 'method': ['LCDM (merger) simulations'], 'model': ['LCDM', 'Osipkov-Merritt formula', 'isotropic NFW model']}
+
+2024-07-16 04:25:29,575 - INFO - Predicted Response:
+assistant
+
+model: LCDM, NFW
+property: radial anisotropy, M/L
+
+2024-07-16 04:25:29,575 - INFO - Predicted Tag:
+{'model': ['LCDM', 'NFW'], 'property': ['radial anisotropy', 'M/L']}
+
+2024-07-16 04:25:31,336 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Thus, the DM model and radial anisotropy can partly explain the low PN VDs, but not in full
+Extractions:
+
+
+2024-07-16 04:25:31,336 - INFO - True Tag:
+{'model': ['DM model'], 'property': ['radial anisotropy']}
+
+2024-07-16 04:25:31,336 - INFO - Predicted Response:
+assistant
+
+model: DM model
+
+2024-07-16 04:25:31,336 - INFO - Predicted Tag:
+{'model': ['DM model']}
+
+2024-07-16 04:25:34,194 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: In an appendix, single integral expressions are derived for the VDs in terms of the tracer density and total mass profiles, for 3 anisotropic models: radial, Osipkov-Merritt, and the model above, for general radial profiles of luminosity density and mass.
+Extractions:
+
+
+2024-07-16 04:25:34,194 - INFO - True Tag:
+{'task': ['single integral expressions are derived'], 'method': ['single integral expressions'], 'property': ['tracer density', 'total mass', 'radial profiles', 'luminosity', 'density', 'mass'], 'model': ['anisotropic models', 'radial', 'Osipkov-Merritt']}
+
+2024-07-16 04:25:34,194 - INFO - Predicted Response:
+assistant
+
+model: anisotropic models, Osipkov-Merritt model
+
+2024-07-16 04:25:34,194 - INFO - Predicted Tag:
+{'model': ['anisotropic models', 'Osipkov-Merritt model']}
+
+2024-07-16 04:25:34,195 - INFO - ##################################################
+2024-07-16 04:25:36,261 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: On the appearance of hyperons in neutron stars
+Extractions:
+
+
+2024-07-16 04:25:36,261 - INFO - True Tag:
+{'object': ['hyperons', 'neutron stars']}
+
+2024-07-16 04:25:36,261 - INFO - Predicted Response:
+assistant
+
+object: hyperons, neutron stars
+
+2024-07-16 04:25:36,261 - INFO - Predicted Tag:
+{'object': ['hyperons', 'neutron stars']}
+
+2024-07-16 04:25:39,536 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: By employing a recently constructed hyperon-nucleon potential the equation of state of \beta-equilibrated and charge neutral nucleonic matter is calculated
+Extractions:
+
+
+2024-07-16 04:25:39,536 - INFO - True Tag:
+{'model': ['hyperon-nucleon potential'], 'property': ['equation of state'], 'object': ['\\\\beta-equilibrated and charge neutral nucleonic matter']}
+
+2024-07-16 04:25:39,536 - INFO - Predicted Response:
+assistant
+
+model: equation of state
+object: hyperon-nucleon potential, nucleonic matter
+
+2024-07-16 04:25:39,536 - INFO - Predicted Tag:
+{'model': ['equation of state'], 'object': ['hyperon-nucleon potential', 'nucleonic matter']}
+
+2024-07-16 04:25:42,592 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: The hyperon-nucleon potential is a low-momentum potential which is obtained within a renormalization group framework
+Extractions:
+
+
+2024-07-16 04:25:42,592 - INFO - True Tag:
+{'model': ['hyperon-nucleon potential', 'renormalization group'], 'property': ['momentum']}
+
+2024-07-16 04:25:42,592 - INFO - Predicted Response:
+assistant
+
+method: renormalization group framework
+object: hyperon-nucleon potential
+
+2024-07-16 04:25:42,592 - INFO - Predicted Tag:
+{'method': ['renormalization group framework'], 'object': ['hyperon-nucleon potential']}
+
+2024-07-16 04:25:44,681 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: Based on the Hartree-Fock approximation at zero temperature the densities at which hyperons appear in neutron stars are estimated
+Extractions:
+
+
+2024-07-16 04:25:44,681 - INFO - True Tag:
+{'model': ['Hartree-Fock approximation'], 'property': ['temperature', 'densities'], 'task': ['the densities at which hyperons appear in neutron stars are estimated'], 'object': ['hyperons', 'neutron stars']}
+
+2024-07-16 04:25:44,681 - INFO - Predicted Response:
+assistant
+
+model: Hartree-Fock approximation
+
+2024-07-16 04:25:44,681 - INFO - Predicted Tag:
+{'model': ['Hartree-Fock approximation']}
+
+2024-07-16 04:25:46,766 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: For several different bare hyperon-nucleon potentials and a wide range of nuclear matter parameters it is found that hyperons in neutron stars are always present
+Extractions:
+
+
+2024-07-16 04:25:46,767 - INFO - True Tag:
+{'model': ['bare hyperon-nucleon potentials'], 'object': ['hyperons', 'neutron stars']}
+
+2024-07-16 04:25:46,767 - INFO - Predicted Response:
+assistant
+
+object: hyperons, neutron stars
+
+2024-07-16 04:25:46,767 - INFO - Predicted Tag:
+{'object': ['hyperons', 'neutron stars']}
+
+2024-07-16 04:25:48,524 - INFO - Prompt:
+The following schema is provided to tag the title and abstract of a given scientific paper as shown in the examples:
+model: a representation of a (scientific) phenomenon using mathematical formalism and/or computational simulation
+task: a specific problem, objective or goal to be accomplished
+dataset: a collection of data, measurements or observations
+field: an academic (sub)discipline
+modality: a class or type of data/observations with similar or the same structure
+method: an approach, technique or procedure to complete a task
+object: an entity that can be studied
+property: a quantitative or qualitative descriptor, or an inherent attribute of an entity, data, modality or method
+instrument: a device or system used for making measurements
+
+Sentence: The polarised emission follows the contours of the strongest of X-ray emission
+Extractions:
+object: polarised emission, X-ray emission
+
+Sentence: This magnetic field strength implies a minimum total energy of the synchrotron radiation of E$_{\textrm{min}} \approx$ 1.8$\times$10$^{48}$ ergs.
+Extractions:
+property: magnetic field strength, energy
+object: synchrotron radiation
+
+Sentence: We present an analysis of a new Australia Telescope Compact Array (ATCA) radio-continuum observation of supernova remnant (SNR) G1.9+0.3, which at an age of $\sim$181$\pm$25 years is the youngest known in the Galaxy
+Extractions:
+dataset: Australia Telescope Compact Array (ATCA) radio-continuum observation
+instrument: Australia Telescope Compact Array (ATCA)
+modality: radio-continuum
+object: supernova remnant (SNR) G1.9+0.3, Galaxy
+property: age
+
+Sentence: It is not difficult for this to occur in inflationary models where quantum fluctuations in a field other than the inflaton contribute to the density perturbations
+Extractions:
+model: inflationary models
+object: quantum fluctuations, inflaton, density perturbations
+modality: density
+
+Sentence: However, an awkward fine tuning seems to be unavoidable.
+Extractions:
+
+Sentence: One possibility is that a trispectrum will be observed without evidence for a non-zero bispectrum
+Extractions:
+property: trispectrum, bispectrum
+
+Sentence: Oxygen abundances for 63 nearby F and G dwarf stars, based on very high resolution spectra ($R\sim215 000$) and high signal-to-noise ($S/N>400$) of the faint forbidden oxygen line at 6300 {\AA}, have been determined
+Extractions:
+object: Oxygen abundances, Oxygen, F, G, dwarf stars, oxygen line
+modality: spectra
+property: signal-to-noise
+
+Sentence: Our findings can be summarized as follows: {\bf 1)} at $\rm [Fe/H]<0$ the oxygen trends in the thin and thick disk are smooth and distinct, indicating their different origins, {\bf 2)} $\rm [O/Fe]$ for the thick disk stars show a turn-over at [Fe/H]$\sim -0.35$, indicating the peak of the enrichment from SNe type Ia to the interstellar medium, {\bf 3)} the thin disk stars show a shallow decrease going from $\rm [Fe/H] \sim -0.7$ to the highest metallicities with no apparent turn-over present indicating a more quiet star formation history, and {\bf 4)} $\rm [O/Fe]$ continues to decrease at $\rm [Fe/H]>0$ without showing the leveling out that previously has been seen.
+Extractions:
+object: oxygen trends, oxygen, disk, thick disk stars, interstellar medium, thin disk stars, star
+property: thin, thick, thick disk, thin disk, metallicities
+
+Sentence: First results from a study into the abundance trends of oxygen in the Galactic thin and thick disks are presented
+Extractions:
+property: abundance trends, thin, thick
+object: oxygen, disks
+
+Sentence: These findings have profound consequences for the mass and radius of neutron stars.
+Extractions:
+
+
+2024-07-16 04:25:48,524 - INFO - True Tag:
+{'property': ['mass', 'radius'], 'object': ['neutron stars']}
+
+2024-07-16 04:25:48,524 - INFO - Predicted Response:
+assistant
+
+object: neutron stars
+
+2024-07-16 04:25:48,524 - INFO - Predicted Tag:
+{'object': ['neutron stars']}
+
+2024-07-16 04:25:48,533 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746
+2024-07-16 04:25:48,534 - INFO - Results saved in: results/eval_random_readable_zoOLWDdW_20240716_040746