T. S. Metcalfe

TL;DR: In this article, the authors describe processing procedures developed by the Kepler Asteroseismic Science Consortium (KASC) to prepare light curves that are optimized for the solar-like oscillating stars in which outliers, jumps and drifts are corrected.

TL;DR: In this article, a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array was used to measure the angular sizes of five main-sequence stars, one subgiant and four red giant stars for which solar-like oscillations have been detected by either Kepler or CoRoT.

TL;DR: A detailed spectroscopic study of 93 solar-type stars that were targets of the NASA/Kepler mission and provided detailed chemical composition of each target is presented in this paper.

TL;DR: In this article, a sample of white dwarfs is selected from SDSS DR3 imaging data using their reduced proper motions, based on improved proper motions from the combined USNO-B combined data, and a luminosity function is constructed covering the range 7 < M_bol < 16.

TL;DR: In this paper, the authors used a variety of independent codes and analyses that attempt to match the asteroseismic and spectroscopic constraints simultaneously to determine both the radius and the age of the subgiant KIC 11026764 with a precision near 1%.