Aguirre, V Silva; Casagrande, Luca; Basu, S; Campante, T. L.; Chaplin, W. J.; Huber, D; Miglio, A; Serenelli, A. M.; Ballot, J; Bedding, T. R.; Christensen-Dalsgaard, J; Weiss, A
Accurately determining the properties of stars is of prime importance for characterizing stellar populations in our Galaxy. The field of asteroseismology has been thought to be particularly successful in such an endeavor for stars in different evolutionary stages. However, to fully exploit its potential, robust methods for estimating stellar parameters are required and independent verification of the results is mandatory. With this purpose, we present a new technique to obtain stellar...[Show more]
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