Installation
About
A pipeline for estimating the stellar age, mass, and radius given observational effective temperature, [Fe/H], and astroseismic parameters. The results are obtained adopting a maximum likelihood technique over a grid of pre-computed stellar models, as described in Valle et al. (2014) doi:10.1051/0004-6361/201322210.
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Maintainer
| Maintainer | Matteo Dell'Omodarme |