We characterize the occurrence rate of planets, ranging in size from 0.5 to 16 R⊕, orbiting
FGK stars with orbital periods from 0.5 to 500 days. Our analysis is based on results from …

Observations of exoplanetary systems provide clues about the intrinsic distribution of
planetary systems, their architectures, and how they formed. We develop a forward …

The angular momentum deficit (AMD) of a planetary system is a measure of its orbital
excitation and a predictor of long-term stability. We adopt the AMD-stability criterion to …

We present robust planet occurrence rates for Kepler planet candidates around M stars for
planet radii Rp= 0.5–4 R⊕ and orbital periods P= 0.5–256 d using the approximate …

We present a new framework to characterize the occurrence rates of planet candidates
identified by Kepler based on hierarchical Bayesian modeling, approximate Bayesian …

The Kepler mission observed thousands of transiting exoplanet candidates around
hundreds of thousands of FGK dwarf stars. He et al. applied forward modeling to infer the …

The thousands of exoplanets identified over the past decade have enabled the study of
exoplanet occurrence rates, which provide an important foundation for the characterization …