Asteroseismic fundamental properties of solar-type stars observed by the NASA Kepler Mission

W. J. Chaplin, S. Basu, D. Huber, A Serenelli, L. Casagrande, V. Silva Aguirre, W. H. Ball, O. L. Creevey, L. Gizon, R. Handberg, C. Karoff, R. Lutz, J. P. Marques, A. Miglio, D. Stello, M. D. Suran, D. Pricopi, T. S. Metcalfe, M. J. P. F. G. Monteiro, J. Molenda-Zakowicz, T. Appourchaux, J. Christensen-Dalsgaard, Y. Elsworth, R. A. Garcia, G. Houdek, H. Kjeldsen, A. Bonanno, T. L. Campante, E. Corsaro, P. Gaulme, S. Hekker, S. Mathur, B. Mosser, C. Regulo, D. Salabert (Submitted on 15 Oct 2013)

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 a survey mode. Stellar properties have been estimated using two global asteroseismic parameters and complementary photometric and spectroscopic data. Homogeneous sets of effective temperatures were available for the entire ensemble from complementary photometry; spectroscopic estimates of T_eff and [Fe/H] were available from a homogeneous analysis of ground-based data on a subset of 87 stars. [Abbreviated version… see paper for full abstract.]

Comments: Accepted for publication in ApJS; 90 pages, 22 figures, 6 tables

Subjects: Solar and Stellar Astrophysics (astro-ph.SR)

Cite as: arXiv:1310.4001 [astro-ph.SR] (or arXiv:1310.4001v1 [astro-ph.SR] for this version)

Submission history From: William Chaplin [v1] Tue, 15 Oct 2013 10:53:45 GMT (5128kb,D) 

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