Stellar CharactEristics Pisa Estimation gRid

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) .


Reference manual

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0.2-4 by Matteo Dell'Omodarme, 10 months ago

Browse source code at

Authors: Matteo Dell'Omodarme [aut, cre] , Giada Valle [aut]

Documentation:   PDF Manual  

Task views: Chemometrics and Computational Physics

GPL (>= 2) license

Depends on MASS, parallel

Suggests lattice

Depended on by SCEPtERbinary.

See at CRAN