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Part 1: Document Description
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Citation |
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Title: |
JJ-model isochrone set: PARSEC, MIST, and BaSTI stellar evolution |
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Identification Number: |
doi:10.11588/data/ZCXHOE |
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Distributor: |
heiDATA |
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Date of Distribution: |
2022-04-11 |
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Version: |
1 |
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Bibliographic Citation: |
Sysoliatina, Kseniia, 2022, "JJ-model isochrone set: PARSEC, MIST, and BaSTI stellar evolution", https://doi.org/10.11588/data/ZCXHOE, heiDATA, V1 |
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Citation |
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Title: |
JJ-model isochrone set: PARSEC, MIST, and BaSTI stellar evolution |
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Identification Number: |
doi:10.11588/data/ZCXHOE |
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Authoring Entity: |
Sysoliatina, Kseniia (Heidelberg University, Astronomisches Rechen-Institut (ARI)) |
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Software used in Production: |
PARSEC, COLIBRI |
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Software used in Production: |
MIST |
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Software used in Production: |
BaSTI |
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Distributor: |
heiDATA |
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Access Authority: |
Sysoliatina, Kseniia |
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Holdings Information: |
https://doi.org/10.11588/data/ZCXHOE |
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Study Scope |
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Keywords: |
Astronomy and Astrophysics |
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Abstract: |
This dataset contains three alternative isochrone grids generated by different stellar evolution codes - PARSEC (Padova), MIST, and BaSTI. Grids cover a wide range of metallicities from approx. -2.6 to +0.5 (60-62 individual metallicities) and ages from 0 to 13 Gyr with a fine step of 50 Myr. Included photometric systems are UBVRIJHK+Gaia_DR2+Gaia_EDR3 (Padova), UBVRI+2MASS+Gaia_DR2+Gaia_EDR3 (MIST), and Gaia_EDR3 (BaSTI). <br> Isochrone grids are part of the python package <a href="https://github.com/askenja/jjmodel">jjmodel</a>. |
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Notes: |
jjmodel on GitHub: <a href="https://github.com/askenja/jjmodel">https://github.com/askenja/jjmodel</a> |
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Methodology and Processing |
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Sources Statement |
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Data Access |
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Citation Requirement: |
If you use these data for the stellar population synthesis with the python code jjmodel, please cite our paper Sysoliatina and Just (2022), in prep. If you use this dataset not with the JJ model, but for your own purposes, cite it as follows: <br> Sysoliatina, Kseniia, 2022, "JJ-model isochrone set: PARSEC, MIST, and BaSTI stellar evolution", <a href="https://doi.org/10.11588/data/ZCXHOE">https://doi.org/10.11588/data/ZCXHOE</a>, heiDATA, V1. <br> <br> Additionally, cite papers of the corresponding stellar evolution groups. <br> PARSEC: <a href="https://ui.adsabs.harvard.edu/abs/2012MNRAS.427..127B/abstract">Bressan et al. (2012)</a>, optionally <a href="https://ui.adsabs.harvard.edu/abs/2013MNRAS.434..488M/abstract">Marigo et al. (2013)</a>, <a href="https://ui.adsabs.harvard.edu/abs/2017ApJ...835...77M/abstract">Marigo et al. (2017)</a> <br> MIST: <a href="https://ui.adsabs.harvard.edu/abs/2016ApJS..222....8D/abstract">Dotter (2016)</a> and <a href="https://ui.adsabs.harvard.edu/abs/2016ApJ...823..102C/abstract">Choi et al. (2016)</a>, optionally some of <a href="https://ui.adsabs.harvard.edu/abs/2011ApJS..192....3P/abstract">Paxton et al. (2011)</a> <a href="https://ui.adsabs.harvard.edu/abs/2013ApJS..208....4P/abstract">Paxton et al. (2013)</a> <a href="https://ui.adsabs.harvard.edu/abs/2015ApJS..220...15P/abstract">Paxton et al. (2015)</a> <a href="https://ui.adsabs.harvard.edu/abs/2018ApJS..234...34P/abstract">Paxton et al. (2018)</a> <br> BaSTI: <a href="https://ui.adsabs.harvard.edu/abs/2018ApJ...856..125H/abstract">Hidalgo et al. (2018)</a> |
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Other Study Description Materials |
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Related Publications |
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Citation |
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Title: |
Sysoliatina and Just (2022), in prep. |
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Bibliographic Citation: |
Sysoliatina and Just (2022), in prep. |
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Label: |
gaiaedr3_basti.zip |
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Notes: |
application/zip |
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Label: |
multiband_mist.zip |
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Text: | |
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Notes: |
application/zip |
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Label: |
multiband_padova.zip |
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Notes: |
application/zip |