Robert C. Morehead

TL;DR: In this paper, the authors report the distribution of planets as a function of planet radius, orbital period, and stellar effective temperature for orbital periods less than 50 days around solar-type (GK) stars.

TL;DR: In this article, the authors report the distribution of planets as a function of planet radius (R_p), orbital period (P), and stellar effective temperature (Teff) for P < 50 day orbits around GK stars.

TL;DR: In this article, the authors characterize the dynamical properties of these candidate multi-planet systems and find that virtually all candidate systems are stable, as tested by numerical integrations that assume a nominal mass-radius relationship.

TL;DR: Kepler spacecraft observations of a single Sun-like star are reported that reveal six transiting planets, five with orbital periods between 10 and 47 days and a sixth planet with a longer period, among the smallest for which mass and size have both been measured.

TL;DR: In this article, Batalha et al. report on the orbital architectures of Kepler systems having multiple-planet candidates identified in the analysis of data from the first six quarters of Kepler data and report that only two pairs of planets in these candidate systems appear to be on Hill-unstable orbits, indicating ~96% of the candidate planetary systems are correctly interpreted as true systems.