Ensemble Asteroseismology with the TRILEGALand the PARAM codesAn estimate of the systematic errors introduced by stellar models
2017
Asteroseismology has provided precise methods for stellar parameters estimation
(e.g. mass, radius and age of stars). Our aim is to quantify systematic errors when
the Bayesian method implemented in the PARAM code is applied with various input
grids of evolutionary tracks. We consider three grids characterized by different
overshooting parameters for convective H-burning cores. Error estimates on the
derived parameters are obtained through simulations of stellar populations with the
TRILEGAL code.
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