Published February 21, 2025 | Version 2.1.2
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Kiauhoku Stellar Evolutionary Model Grids

  • 1. ROR icon University of Florida

Description

Stellar evolutionary model grids for use with Python Kiauhoku package (presented by Claytor et al. 2020). This dataset contains models from MIST, YREC, GARSTEC, and Dartmouth projects.

Model Grids

fastlaunch

Originally presented by Claytor et al. (2020). Computed using the Yale Rotating stellar Evolution Code (YREC, Pinsonneault et al. 1989) with rotational evolution computed separately using the magnetic braking law of van Saders and Pinsonneault (2013) under "fast launch" condition of Pinit ~ 8 days.

slowlaunch

Originally presented by Claytor et al. (2020). Computed using the Yale Rotating stellar Evolution Code (YREC, Pinsonneault et al. 1989) with rotational evolution computed separately using the magnetic braking law of van Saders and Pinsonneault (2013) under "slow launch" condition of Pinit ~ 13 days.

rocrit

Originally presented by Claytor et al. (2020). Computed using the Yale Rotating stellar Evolution Code (YREC, Pinsonneault et al. 1989) with rotational evolution computed separately using the stalled magnetic braking law of van Saders et al. (2016) under "fast launch" condition of Pinit ~ 8 days.

mist

Evolutionary tracks from the MESA Isochrones and Stellar Tracks (MIST, Choi et al. 2016). Computed using Modules for Experiments in Stellar Astrophysics (MESA, Paxton et al. 2010).

yrec

Originally presented by Tayar et al. (2022). Computed using the Yale Rotating stellar Evolution Code (YREC, Pinsonneault et al. 1989).

dartmouth

Originally presented by Dotter et al. (2008). Models from the Dartmouth Stellar Evolution Program (DSEP).

garstec

Originally presented by Serenelli et al. (2013). Computed using the Garching Stellar Evolution Code (GARSTEC, Weiss & Schlattl 2008).

Notes

v. 2.1.2 Resampled EEPs for YREC, GARSTEC, and Dartmouth grids, following Morales et al. (2025).

v. 2.1.1 [DEPRECATED - accidentally deleted old files]

v. 2.1.0 added the full available MIST EEP tracks, rather than just a subset. 

v. 2.0.3 fixed a minor bug in the YREC EEP tracks for M/Msun >= 1.8 that mistook the TRGB as the RGB bump. Removed the bump as an EEP; now all tracks (save one, M/Msun = 0.7, [Z/X] = +0.5) correctly reach the TRGB. fixed critical bug from v. 2.0.2.

v. 2.0.2 [DEPRECATED: critical bug in the yrec_eep.tar.gz file, where kiauhoku would download it, not realize it downloaded, and infinitely try to download again. This bug is only present in v 2.0.2]

v. 2.0.1 updated Dartmouth and Garstec EEP grids to extend to RGBTip.

v. 2.0 updated directory structure for compatibility with kiauhoku v. 2.0.

v. 1.3 src and eep files provided for individual model grids.

v. 1.2 bug fixed in Dartmouth (DSEP) grid that affected placement of Terminal Age Main-Sequence EEP in ~25% of tracks.

v. 1.1 grids are identical, but added separately downloadable interpolators and grids, as well as an option for bulk download.

Files

Files (7.8 GB)

Name Size Download all
md5:0ce83def4548b8d3e4764733b8567fee
20.2 MB Download
md5:c4634fd2260ced2c8e456d7641245595
2.9 MB Download
md5:04093377c0d3452b41559a468c5f8f91
5.9 MB Download
md5:e096a0d8ae08714aa5c07eb272d7199f
134.7 MB Download
md5:78fd66271c9d32df14f76598d14020d6
1.1 GB Download
md5:4520878cd590056f6388ecce48f8e947
873.7 MB Download
md5:aed798b915c478b6bc07275da3d37167
3.7 MB Download
md5:7df26f88c425d69777bb7f4a3e3bd213
11.3 MB Download
md5:e26a0dbb0aa2b4d3586419b4fc14b3d0
19.7 MB Download
md5:ef01ea924b800812bfc085f90141760c
1.3 GB Download
md5:c0846131f9efc6c6197a11f36e5458fa
131.0 MB Download
md5:27339ff185616b450ca7a80e163e0da4
1.1 GB Download
md5:fa9adab211e354b48f7ab3c0a19461fe
859.2 MB Download
md5:a8d217feaa3941b8e27ef63611a8a698
132.0 MB Download
md5:636bac9f5d2ddd8d7b47884f331b4986
1.1 GB Download
md5:b40adee74042644e9416ec472e9d1e4c
867.7 MB Download
md5:fad36e2738e0175528ff4b4da6878f46
10.5 MB Download
md5:391f05de8d2fe6b25be4bc8de2b2d815
62.5 MB Download
md5:8940244d0b240d33b41a0037cbd6f3bb
102.8 MB Download

Additional details

References

  • Choi, J. et al. 2016a, ApJ, 823, 102
  • Claytor, Z. R. et al. 2020, ApJ, 888, 43
  • Dotter, A. 2016, ApJS, 222, 8
  • Paxton, B. et al. 2010, Astrophysics Source Code Library, record ascl:1010.083
  • Pinsonneault, M. H. et al. 1989, ApJ, 338, 424
  • Serenelli, A. M. et al. 2013, MNRAS, 429, 3645
  • van Saders, J. L. & Pinsonneault, M. H. 2013, ApJ, 776, 67
  • van Saders, J. L. et al. 2016, Nature, 529, 181
  • Weiss, A., & Schlattl, H. 2008, Ap&SS, 316, 99