activity
20022024
most citedA continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion

979 citations · 17.5k across the 125 of their papers we have counts for

collaborators

126 papers

astro-ph.EP2024

A Comprehensive Analysis Spitzer 4.5 m Phase Curve of Hot Jupiters

Lisa Dang, Taylor J. Bell, Ying +19

Although exoplanetary science was not initially projected to be a substantial part of the Spitzer mission, its exoplanet observations set the stage for current and future surveys w…

astro-ph.EP2022★ 15 cited

Particle deposition on the saturnian satellites from ephemeral cryovolcanism on Enceladus

Naoyuki Hirata, Hideaki Miyamoto, Adam P. Showman

The geologically active south pole of Enceladus generates a plume of micron-sized particles, which likely form Saturn's tenuous E-ring extending from the orbit of Mimas to Titan. I…

astro-ph.EP2022★ 37 cited

A New Analysis of 8 Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b

Erin May, Kevin Stevenson, Jacob Bean +16

With over 30 phase curves observed during the warm Spitzer mission, the complete data set provides a wealth of information relating to trends and three-dimensional properties of ho…

astro-ph.EP2022★ 6 cited

Influences of internal forcing on atmospheric circulations of irradiated giant planets

Yuchen Lian, Adam P. Showman, Xianyu Tan +1

Close-in giant planets with strong stellar irradiation show atmospheric circulation patterns with strong equatorial jets and global-scale stationary waves. So far, almost all model…

astro-ph.EP2021★ 14 cited

Thermal Phase Curves of XO-3b: an Eccentric Hot Jupiter at the Deuterium Burning Limit

Lisa Dang, Taylor J. Bell, Nicolas B. Cowan +15

We report \textit{Spitzer} full-orbit phase observations of the eccentric hot Jupiter XO-3b at 3.6 and 4.5 m. Our new eclipse depth measurements of ppm at 3.6 …

astro-ph.EP2021★ 3 cited

Spitzer phase curve observations and circulation models of the inflated ultra-hot Jupiter WASP-76b

Erin M. May, Thaddeus D. Komacek, Kevin B. Stevenson +15

The large radii of many hot Jupiters can only be matched by models that have hot interior adiabats, and recent theoretical work has shown that the interior evolution of hot Jupiter…