SCEPtER 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.
|Author||Matteo Dell'Omodarme [aut, cre], Giada Valle [aut]|
|Date of publication||2015-01-05 16:33:07|
|Maintainer||Matteo Dell'Omodarme <[email protected]>|
|License||GPL (>= 2)|
|Package repository||View on CRAN|
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