Chaplin, W J; Basu, S; Huber, D; Serenelli, Aldo; Casagrande, Luca; Silva Aguirre, V; Ball, W.H.; Creevey, O L; Gizon, L; Handberg, R.; Karoff, C.
We use asteroseismic data obtained by the NASA Kepler mission to estimate the fundamental properties of more than 500 main-sequence and sub-giant stars. Data obtained during the first 10 months of Kepler science operations were used for this work, when these solar-type targets were observed for one month each in survey mode. Stellar properties have been estimated using two global asteroseismic parameters and complementary photometric and spectroscopic data. Homogeneous sets of effective...[Show more]
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