activity
20182024
most citedHow drifting and evaporating pebbles shape giant planets I: Heavy element content and atmospheric C/O

174 citations · 470 across the 20 of their papers we have counts for

collaborators
Showing 2022Show all

5 papers · 1 filter

astro-ph.EP2022★ 26 cited

Clouds form on the hot Saturn JWST ERO target WASP-96b

Dominic Samra, Christiane Helling, Katy Chubb +3

WASP-96b is a hot Saturn exoplanet, with an equilibrium temperature well within the regime of thermodynamically expected extensive cloud formation. Prior observations with Hubble/W…

astro-ph.EP2022★ 22 cited

No evidence for radius inflation in hot Jupiters from vertical advection of heat

Aaron David Schneider, Ludmila Carone, Leen Decin +2

Understanding the radiative-dynamical coupling between upper photosphere and deeper atmosphere is a key in understanding the abnormal large radii of hot Jupiters. One needs very lo…

astro-ph.EP2022★ 38 cited

How drifting and evaporating pebbles shape giant planets III: The formation of WASP-77A b and Boötis b

Bertram Bitsch, Aaron David Schneider, Laura Kreidberg

Atmospheric abundances are thought to constrain the planet formation pathway, because different species evaporate at different temperatures leaving distinct signatures in the accre…

astro-ph.EP2022★ 2 cited

Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions

Paul Mollière, Tamara Molyarova, Bertram Bitsch +13

Constraining planet formation based on the atmospheric composition of exoplanets is a fundamental goal of the exoplanet community. Existing studies commonly try to constrain atmosp…

astro-ph.EP2022

Exploring the deep atmospheres of HD 209458b and WASP-43b using a non-gray general circulation model

Aaron David Schneider, Ludmila Carone, Leen Decin +5

Simulations with a 3D general circulation model (GCM) suggest that one potential driver behind the observed radius inflation in hot Jupiters may be the downward advection of energy…