Kepler asteroseismic LEGACY sample. I. Oscillations

Here we analyze a sample of 66 Kepler main-sequence stars showing solar-like oscillations as part of the Kepler seismic LEGACY project. We use Kepler short-cadence data, of which each star has at least 12 months, to create frequency-power spectra optimized for asteroseismology.

For each star, we identify its modes of oscillation and extract parameters such as frequency, amplitude, and line width using a Bayesian Markov chain Monte Carlo "peak-bagging" approach. We report the extracted mode parameters for all 66 stars, as well as derived quantities such as frequency difference ratios, the large and small separations {Delta}{nu} and {delta}{nu}_02_; the behavior of line widths with frequency and line widths at {nu}_max_ with T_eff_, for which we derive parametrizations; and behavior of mode visibilities.