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 2023Show all

5 papers · 1 filter

astro-ph.EP2023★ 1 cited

Harnessing machine learning for accurate treatment of overlapping opacity species in general circulation models

Aaron David Schneider, Paul Mollière, Gilles Louppe +4

To understand high precision observations of exoplanets and brown dwarfs, we need detailed and complex general circulation models (GCMs) that incorporate hydrodynamics, chemistry,…

astro-ph.EP2023★ 3 cited

Constraining the formation history of the HAT-P-11 system by atmospheric abundances

Lena Chatziastros, Bertram Bitsch, Aaron David Schneider

The chemical fingerprint of a planet reveals information about its formation history regarding when and where it formed. The water content of a planet can help to constrain its for…

astro-ph.EP2023★ 12 cited

Photodissociation and induced chemical asymmetries on ultra-hot gas giants. A case study of HCN on WASP-76 b

Robin Baeyens, Jean-Michel Désert, Annemieke Petrignani +2

Recent observations have resulted in the detection of chemical gradients on ultra-hot gas giants. Notwithstanding their high temperature, chemical reactions in ultra-hot atmosphere…

astro-ph.EP2023★ 11 cited

Evidence of Radius Inflation in Radiative GCM Models of WASP-76b due to the Advection of Potential Temperature

Felix Sainsbury-Martinez, Pascal Tremblin, Aaron David Schneider +6

Understanding the discrepancy between the radii of observed hot Jupiters and standard 'radiative-convective' models remains a hotly debated topic in the exoplanet community. One me…

astro-ph.EP2023★ 4 cited

WASP-39b: exo-Saturn with patchy cloud composition, moderate metallicity, and underdepleted S/O

Ludmila Carone, David A. Lewis, Dominic Samra +2

WASP-39b is one of the first extrasolar giant gas planets that has been observed within the JWST ERS program. Fundamental properties that may enable the link to exoplanet formation…