Lund, M. N.; Silva Aguirre, V.; Davies, G. R.; Chaplin, W. J.; Christensen-Dalsgaard, J.; Houdek, Gunter; White, Timothy R.; Bedding, T. R.; Ball, W. H.; Huber, D.; Casagrande, Luca
The advent of space-based missions like Kepler has revolutionized the study of solar-type stars, particularly through the measurement and modeling of their resonant modes of oscillation. 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...[Show more]
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