activity
20172026
most citedA Sub-Neptune Exoplanet with a Low-Metallicity Methane-Depleted Atmosphere and Mie-Scattering Clouds

238 citations · 1.6k across the 62 of their papers we have counts for

collaborators
Showing 2019Show all

6 papers · 1 filter

astro-ph.EP201981 cited

Detection of ionized calcium in the atmosphere of the ultra-hot Jupiter KELT-9b

Jake D. Turner, Ernst J. W. de Mooij, Ray Jayawardhana +6

With a day-side temperature in excess of 4500K, comparable to a mid-K-type star, KELT-9b is the hottest planet known. Its extreme temperature makes KELT-9b a particularly interesti…

astro-ph.EP2019

Water Vapor and Clouds on the Habitable-Zone Sub-Neptune Exoplanet K2-18b

Björn Benneke, Ian Wong, Caroline Piaulet +13

Results from the Kepler mission indicate that the occurrence rate of small planets ( ) in the habitable zone of nearby low-mass stars may be as high as 80%. Despite t…

astro-ph.EP2019238 cited

A Sub-Neptune Exoplanet with a Low-Metallicity Methane-Depleted Atmosphere and Mie-Scattering Clouds

Björn Benneke, Heather A. Knutson, Joshua Lothringer +15

With no analogues in the Solar System, the discovery of thousands of exoplanets with masses and radii intermediate between Earth and Neptune was one of the big surprises of exoplan…

astro-ph.EP201911 cited

The Need for Laboratory Measurements and Ab Initio Studies to Aid Understanding of Exoplanetary Atmospheres

Jonathan J. Fortney, Tyler D. Robinson, Shawn Domagal-Goldman +85

We are now on a clear trajectory for improvements in exoplanet observations that will revolutionize our ability to characterize their atmospheric structure, composition, and circul…

astro-ph.EP201973 cited

The Influence of Host Star Spectral Type on Ultra-Hot Jupiter Atmospheres

Joshua D. Lothringer, Travis S. Barman

Ultra-hot Jupiters are the most highly irradiated gas giant planets, with equilibrium temperatures from 2000 to over 4000 K. Ultra-hot Jupiters are amenable to characterization due…

astro-ph.SR201922 cited

Unusual Isotopic Abundances in a Fully-Convective Stellar Binary

I. J. M. Crossfield, J. D. Lothringer, B. Flores +6

Low-mass M dwarfs represent the most common outcome of star formation, but their complex emergent spectra hinder detailed studies of their composition and initial formation. The me…