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Aaron David Schneider

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP2
  • astro-ph.IM1
ORCID 0000-0002-1448-0303

identity via Semantic Scholar / OpenAlex

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

38 citations · 43 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.EP2024★ 5 cited

Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b

Taylor J. Bell, Nicolas Crouzet, Patricio E. Cubillos +80

Hot Jupiters are among the best-studied exoplanets, but it is still poorly understood how their chemical composition and cloud properties vary with longitude. Theoretical models pr…

astro-ph.IM2024

chemcomp: Modeling the chemical composition of planets formed in protoplanetary disks

Aaron David Schneider, Bertram Bitsch

Future observations of exoplanets will hopefully reveal detailed constraints on planetary compositions. Recently, we have developed and introduced chemcomp (Schneider & Bitsch 2021…

astro-ph.EP2022★ 38 cited

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

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.