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Wilson, P. Eggenberger, P. Gaulme, R. A. Garcia, R. Handberg, R. L. Gilliland, R. Trampedach, R. Ventura, R. W. Noyes, S. Basu, S. Hekker, S.Mathis, S. Mathur, S. T. Fletcher, T. Appourchaux, T. L. Campante, T. R. Bedding, T. Roca Cortes, T. S. Metcalfe, W. J. Chaplin, Y. Elsworth","submitted_at":"2010-05-04T12:48:35Z","abstract_excerpt":"We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5d of science operations, reveal high signal-to-noise solar-like oscillation spectra in all three stars: About 20 modes of oscillation can clearly be distinguished in each star. 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