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Table A.1.

Input parameters and asteroseismically determined parameters for the 490 analysed γ Dor stars.

Name Unit Description
KIC - KIC ID
RA deg Right ascension from Gaia DR3
Dec deg Declination from Gaia DR3
Lum L Photometric Luminosity (L)
err_Lum L Uncertainty on photometric Luminosity
Teff K Effective temperature from Gaia DR3 (Teff)
err_Teff K Uncertainty on effective temperature
Pi0 s Buoyancy travel time from Li et al. (2020)0)
errl_Pi0 s Lower uncertainty on Π0 from Li et al. (2020)
erru_Pi0 s Upper uncertainty on Π0 from Li et al. (2020)
frot d−1 Near-core rotation rate from Li et al. (2020)rot)
errl_frot d−1 Lower uncertainty on Ωrot from Li et al. (2020)
erru_frot d−1 Upper uncertainty on Ωrot from Li et al. (2020)
Xc’ - Normalised core hydrogen mass fraction ()
errl_Xc’ - Lower uncertainty on
erru_Xc’ - Upper uncertainty on
age Gyr Asteroseismic age (t)
errl_age Gyr Lower uncertainty on age
erru_age Gyr Upper uncertainty on age
mass M Asteroseismic mass (M)
errl_mass M Lower uncertainty on mass
erru_mass M Upper uncertainty on mass
radius R Asteroseismic radius (R)
errl_radius R Lower uncertainty on radius
erru_radius R Upper uncertainty on radius
vvcrit - Ratio of current rotation rate to critical rotation rate (v/vcrit)
MIST_age_TAMS Gyr Age of rotating MIST track at TAMS (tr)
NR_MIST_age_TAMS Gyr Age of non-rotating MIST track at TAMS (tnr)
TAMS_frac - Fraction of rotating to non-rotating age at TAMS (tr/tnr)
MIST_age_TRGB Gyr Age of rotating MIST track at TRGB (tr)
NR_MIST_age_TRGB Gyr Age of non-rotating MIST track at TRGB (tnr)
TRGB_frac - Fraction of rotating to non-rotating age at TRGB (tr/tnr)
MIST_age_ZAHeB Gyr Age of rotating MIST track at ZAHeB (tr)
NR_MIST_age_ZAHeB Gyr Age of non-rotating MIST track at ZAHeB tnr)
ZAHeB_frac - Fraction of rotating to non-rotating age at ZAHeB (tr/tnr)
MIST_age_TAHeB Gyr Age of rotating MIST track at TAHeB (tr)
NR_MIST_age_TAHeB Gyr Age of non-rotating MIST track at TAHeB (tnr)
TAHeB_frac - Fraction of rotating to non-rotating age at TAHeB (tr/tnr)

Notes. The full table is available at the CDS.

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