T. S. Metcalfe

TL;DR: In this paper, an analysis of three months of nearly uninterrupted photometry of 16 Cyg A and B from the Kepler space telescope is presented, including a clear detection of octupole (l=3) modes in both stars.

TL;DR: In this article, the authors used previously published asteroseismic and spectroscopic data sets to provide a uniform analysis of 42 solar-type Kepler targets from AMP and found that fitting the individual frequencies typically doubled the precision of the asteroseismsic radius, mass, and age compared to grid-based modeling of the global oscillation properties, and improved the radius and mass by about a factor of three over empirical scaling relations.

TL;DR: In this article, preliminary asteroseismic results from Kepler on three G-type stars are presented, 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 may be clearly distinguished in each star.

TL;DR: In this article, the authors used photometric observations of solar-type stars, made by the NASA Kepler Mission, to conduct a statistical study of the impact of stellar surface activity on the detectability of solarlike oscillations.

TL;DR: In this paper, the authors outline how to make an estimate of the detectability of solar-like oscillations in any given Kepler target, using rough estimates of the temperature and radius, and the Kepler apparent magnitude.