BAGEMASS: Bayesian age and mass estimates for transiting planet host stars
Abstract
BAGEMASS calculates the posterior probability distribution for the mass and age of a star from its observed mean density and other observable quantities using a grid of stellar models that densely samples the relevant parameter space. It is written in Fortran and requires FITSIO (ascl:1010.001).
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- August 2017
- Bibcode:
- 2017ascl.soft08010M
- Keywords:
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- Software