The planet candidates discovered by the Kepler mission provide a rich sample to constrain
the architectures and relative inclinations of planetary systems within approximately 0.5 AU …

About one-third of the∼ 1200 transiting planet candidates detected in the first four months of
Kepler data are members of multiple candidate systems. There are 115 target stars with two …

We 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 reported by …

The Kepler mission has detected dozens of compact planetary systems with more than four
transiting planets. This sample provides a collection of close-packed planetary systems with …

The Kepler mission has detected thousands of planetary systems with one to seven
transiting planets packed within 0.7 au from their host stars. There is an apparent excess of …

We study the orbital architecture of multi-planet systems detected by the Kepler transit
mission using N-body simulations, focusing on the orbital spacing between adjacent planets …

We present and discuss five candidate exoplanetary systems identified with the Kepler
spacecraft. These five systems show transits from multiple exoplanet candidates. Should …

During its five-year mission, the Kepler spacecraft has uncovered a diverse population of
planetary systems with orbital configurations ranging from single-transiting planets to …

We investigated the underlying architecture of planetary systems by deriving the distribution
of planet multiplicity (number of planets) and the distribution of orbital inclinations based on …

Early analyses of exoplanet statistics from the Kepler mission revealed that a model
population of multiplanet systems with low mutual inclinations (∼ 1–2) adequately describes …