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A. Garcia, R. Handberg, R. L. Gilliland, R. Schonrich, S. Basu, S. D Kawaler, S. G. Sousa, S. Hekker, S. Mathur, T. Appourchaux, T. L. Campante, T. R. Bedding, T. R. White, T. S. Metcalfe, V. Silva Aguirre, W. J. Chaplin, Y. Elsworth","submitted_at":"2011-08-09T20:00:01Z","abstract_excerpt":"Asteroseismology of solar-type stars has entered a new era of large surveys with the success of the NASA \\textit{Kepler} mission, which is providing exquisite data on oscillations of stars across the Hertzprung-Russell (HR) diagram. From the time-series photometry, the two seismic parameters that can be most readily extracted are the large frequency separation ($\\Delta\\nu$) and the frequency of maximum oscillation power ($\\nu_\\mathrm{max}$). After the survey phase, these quantities are available for hundreds of solar-type stars. 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