activity
20182026
most citedIdentification of carbon dioxide in an exoplanet atmosphere

193 citations · 1.4k across the 43 of their papers we have counts for

collaborators
Showing 2021Show all

5 papers · 1 filter

astro-ph.EP2021

All along the line of sight: a closer look at opening angles and absorption regions in the atmospheres of transiting exoplanets

Joost P. Wardenier, Vivien Parmentier, Elspeth K. H. Lee

Transmission spectra contain a wealth of information about the atmospheres of transiting exoplanets. However, large thermal and chemical gradients along the line of sight can lead…

astro-ph.EP2021★ 56 cited

3D radiative-transfer for exoplanet atmospheres. gCMCRT: a GPU accelerated MCRT code

Elspeth K. H. Lee, Joost P. Wardenier, Bibiana Prinoth +10

Radiative-transfer (RT) is a key component for investigating atmospheres of planetary bodies. With the 3D nature of exoplanet atmospheres being important in giving rise to their ob…

astro-ph.EP2021★ 140 cited

A Comparative Study of Atmospheric Chemistry with VULCAN

Shang-Min Tsai, Matej Malik, Daniel Kitzmann +4

We present an update of the open-source photochemical kinetics code VULCAN (Tsai et al. 2017; https://github.com/exoclime/VULCAN) to include C-H-N-O-S networks and photochemistry.…

astro-ph.EP2021★ 60 cited

Simulating gas giant exoplanet atmospheres with Exo-FMS: Comparing semi-grey, picket fence and correlated-k radiative-transfer schemes

Elspeth K. H. Lee, Vivien Parmentier, Mark Hammond +5

Radiative-transfer (RT) is a fundamental part of modelling exoplanet atmospheres with general circulation models (GCMs). An accurate RT scheme is required for estimates of the atmo…

astro-ph.EP2021★ 100 cited

Decomposing the Iron Cross-Correlation Signal of the Ultra-Hot Jupiter WASP-76b in Transmission using 3D Monte-Carlo Radiative Transfer

Joost P. Wardenier, Vivien Parmentier, Elspeth K. H. Lee +2

Ultra-hot Jupiters are tidally locked gas giants with dayside temperatures high enough to dissociate hydrogen and other molecules. Their atmospheres are vastly non-uniform in terms…