activity
20182022
most citedGrowth Model Interpretation of Planet Size Distribution

591 citations · 1.1k across the 9 of their papers we have counts for

collaborators

15 papers

astro-ph.EP20219 cited

Zodiacal Exoplanets in Time (ZEIT) XII: A Directly-Imaged Planetary-Mass Companion to a Young Taurus M Dwarf Star

E. Gaidos, T. Hirano, A. L. Kraus +21

We report the discovery of a resolved (0".9) substellar companion to a member of the 1-5 Myr Taurus star-forming region. The host star (2M0437) is a single mid-M type ($T_{eff}\app…

astro-ph.EP202145 cited

Slow Cooling and Fast Reinflation for Hot Jupiters

Daniel P. Thorngren, Jonathan J. Fortney, Eric D. Lopez +2

The unexpectedly large radii of hot Jupiters are a longstanding mystery whose solution will provide important insights into their interior physics. Many potential solutions have be…

astro-ph.SR2021

The Stars Kepler Missed: Investigating the Kepler Target Selection Function Using Gaia DR2

Linnea M. Wolniewicz, Travis A. Berger, Daniel Huber

The Kepler Mission revolutionized exoplanet science and stellar astrophysics by obtaining highly precise photometry of over 200,000 stars over 4 years. A critical piece of informat…

astro-ph.EP2020180 cited

The Occurrence of Rocky Habitable Zone Planets Around Solar-Like Stars from Kepler Data

Steve Bryson, Michelle Kunimoto, Ravi K. Kopparapu +79

We present occurrence rates for rocky planets in the habitable zones (HZ) of main-sequence dwarf stars based on the Kepler DR25 planet candidate catalog and Gaia-based stellar prop…

astro-ph.EP2020185 cited

The Gaia-Kepler Stellar Properties Catalog. II. Planet Radius Demographics as a Function of Stellar Mass and Age

Travis A. Berger, Daniel Huber, Eric Gaidos +2

Studies of exoplanet demographics require large samples and precise constraints on exoplanet host stars. Using the homogeneous Kepler stellar properties derived using Gaia Data Rel…

astro-ph.SR202046 cited

Exploring the evolution of stellar rotation using Galactic kinematics

Ruth Angus, Angus Beane, Adrian M. Price-Whelan +9

The rotational evolution of cool dwarfs is poorly constrained after around 1-2 Gyr due to a lack of precise ages and rotation periods for old main-sequence stars. In this work we u…