1 code implementation • 7 Feb 2020 • Danley C. Hsu, Eric B. Ford, Ryan Terrien
We caution that occurrence rate estimates for Kepler M stars are sensitive to the choice of prior due to the small sample of target stars and planet candidates.
Earth and Planetary Astrophysics Solar and Stellar Astrophysics
2 code implementations • 4 Feb 2019 • Danley C. Hsu, Eric B. Ford, Darin Ragozzine, Keir Ashby
We characterize the occurrence rate of planets, ranging in size from 0. 5-16 R$_\oplus$, orbiting FGK stars with orbital periods from 0. 5-500 days.
Earth and Planetary Astrophysics