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20202025
most citedThe California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age

133 citations · 661 across the 31 of their papers we have counts for

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Showing 2022Show all

9 papers · 1 filter

astro-ph.EP2022★ 72 cited

TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain

Fei Dai, Kento Masuda, Corey Beard +60

Convergent disk migration has long been suspected to be responsible for forming planetary systems with a chain of mean-motion resonances (MMR). Dynamical evolution over time could…

astro-ph.EP2022★ 38 cited

The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets

Samuel W. Yee, Joshua N. Winn, Joel D. Hartman +83

NASA's Transiting Exoplanet Survey Satellite (TESS) mission promises to improve our understanding of hot Jupiters by providing an all-sky, magnitude-limited sample of transiting ho…

astro-ph.EP2022★ 40 cited

TOI-561 b: A Low Density Ultra-Short Period "Rocky" Planet around a Metal-Poor Star

Casey Brinkman, Lauren M. Weiss, Fei Dai +22

TOI-561 is a galactic thick disk star hosting an ultra-short period (0.45 day orbit) planet with a radius of 1.37 R, making it one of the most metal-poor ([Fe/H] = -0.41…

astro-ph.EP2022★ 15 cited

TESS-Keck Survey XIV: Two giant exoplanets from the Distant Giants Survey

Judah E. Van Zandt, Erik A. Petigura, Mason MacDougall +42

We present the Distant Giants Survey, a three-year radial velocity (RV) campaign to measure P(DG|CS), the conditional occurrence of distant giant planets (DG; M_p ~ 0.3 - 13 M_J, P…

astro-ph.EP2022★ 7 cited

The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272

Mason G. MacDougall, Erik A. Petigura, Tara Fetherolf +58

We report the discovery of an eccentric hot Neptune and a non-transiting outer planet around TOI-1272. We identified the eccentricity of the inner planet, with an orbital period of…

astro-ph.EP2022★ 12 cited

Implicit biases in transit models using stellar pseudo-density

Gregory J. Gilbert, Mason G. MacDougall, Erik A. Petigura

The transit technique is responsible for the majority of exoplanet discoveries to date. Characterizing these planets involves careful modeling of their transit profiles. A common t…

astro-ph.EP2022★ 20 cited

Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant

Isabel Angelo, Smadar Naoz, Erik Petigura +4

Highly eccentric orbits are one of the major surprises of exoplanets relative to the Solar System and indicate rich and tumultuous dynamical histories. One system of particular int…

astro-ph.EP2022

The TESS-Keck Survey. XI. Mass Measurements for Four Transiting sub-Neptunes orbiting K dwarf TOI-1246

Emma V. Turtelboom, Lauren M. Weiss, Courtney D. Dressing +78

Multi-planet systems are valuable arenas for investigating exoplanet architectures and comparing planetary siblings. TOI-1246 is one such system, with a moderately bright K dwarf (…

astro-ph.EP2022★ 133 cited

The California-Kepler Survey. X. The Radius Gap as a Function of Stellar Mass, Metallicity, and Age

Erik A. Petigura, James G. Rogers, Howard Isaacson +10

In 2017, the California-Kepler Survey (CKS) published its first data release (DR1) of high-resolution optical spectra of 1305 planet hosts. Refined CKS planet radii revealed that s…