Published October 4, 2024 | Version v1
Software Open

Estimates of (convective core) masses, radii, and relative ages for ∼14,000 Gaia-discovered gravity-mode pulsators monitored by TESS

Authors/Creators

  • 1. ROR icon Institut de Recherche en Astrophysique et Planétologie
  • 2. ROR icon KU Leuven
  • 3. ROR icon University of Sydney

Description

Files included:

  • MESA r24.03.1 inlist.
  • MESA run_star_extras for rotational mixing.
  • Python script for modelling stars with CNF.
  • Trained CNF for Z = 0.0045 and Z = 0.014. (trained_flow_fullset_logR_Z*_Mext.pth)
  • Relevant parameters of MESA grids used to train CNFs. (grid_Gaia_Z*_ext.pkl)
  • Maximum likelihood estimates of mass, Xc/X, core mass and radius + GSP-Phot Teff and luminosity. (MLE_flow_fullset_logR_Z*_p0.2_68per_inflated_errors3_KDE_master_Npeaks2.pkl)

Files

Files (110.3 MB)

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md5:83a94db618398a7c6f2ab68981115892
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Additional details

Funding

Agence Nationale de la Recherche
MASSIF ANR-21-CE31-0018-02
KU Leuven
PARADISE C16/18/005
European Research Council
4D-STAR 101071505