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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>.
Package details |
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Author | Matteo Dell'Omodarme [aut, cre], Giada Valle [aut] |
Maintainer | Matteo Dell'Omodarme <mattdell@fastmail.fm> |
License | GPL (>= 2) |
Version | 0.2-4 |
Package repository | View on CRAN |
Installation |
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