activity
20122022
most citedKepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the Habitable Zone

255 citations · 1.4k across the 23 of their papers we have counts for

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39 papers · 1 filter

astro-ph.EP20223 cited

The Exoplanet Modeling and Analysis Center at NASA Goddard

Joe P. Renaud, Eric Lopez, Jonathan Brande +8

The Exoplanet Modeling and Analysis Center (EMAC) at NASA Goddard Space Flight Center is a web-based catalog, repository, and integration platform for modeling and analysis resourc…

astro-ph.EP2021

The sub-Neptune desert and its dependence on stellar type: Controlled by lifetime X-ray irradiation

George D. McDonald, Laura Kreidberg, Eric Lopez

Short-period sub-Neptunes with substantial volatile envelopes are among the most common type of known exoplanets. However, recent studies of the Kepler population have suggested a…

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.EP202085 cited

An Ultra-Hot Neptune in the Neptune desert

James S. Jenkins, Matías R. Díaz, Nicolás T. Kurtovic +81

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the…

astro-ph.EP2020

TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert

Jennifer A. Burt, Louise D. Nielsen, Samuel N. Quinn +54

We report the detection of a transiting hot Neptune exoplanet orbiting TOI-824 (SCR J1448-5735), a nearby (d = 64 pc) K4V star, using data from the \textit{Transiting Exoplanet Sur…

astro-ph.EP202045 cited

TOI-1235 b: a keystone super-Earth for testing radius valley emergence models around early M dwarfs

Ryan Cloutier, Joseph E. Rodriguez, Jonathan Irwin +85

Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of the…