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Spitzer Phase Curve Constraints for WASP-43b at 3.6 and 4.5 microns
Kevin B. Stevenson, Michael R. Line, Jacob L. Bean +6
Previous measurements of heat redistribution efficiency (the ability to transport energy from a planet's highly irradiated dayside to its eternally dark nightside) show considerabl…
The Impact of Non-Uniform Thermal Structure on the Interpretation of Exoplanet Emission Spectra
Y. Katherina Feng, Michael R. Line, Jonathan J. Fortney +4
The determination of atmospheric structure and molecular abundances of planetary atmospheres via spectroscopy involves direct comparisons between models and data. While varying in…
HELIOS: An Open-source, GPU-accelerated Radiative Transfer Code For Self-consistent Exoplanetary Atmospheres
Matej Malik, Luc Grosheintz, João M. Mendonça +10
We present the open-source radiative transfer code named HELIOS, which is constructed for studying exoplanetary atmospheres. In its initial version, the model atmospheres of HELIOS…
No Thermal Inversion and a Solar Water Abundance for the Hot Jupiter HD209458b from HST WFC3 Emission Spectroscopy
Michael R. Line, Kevin B. Stevenson, Jacob Bean +6
The nature of the vertical thermal structure of hot Jupiter atmospheres is one of the key questions raised by the characterization of transiting exoplanets over the last decade. Th…
Transiting Exoplanet Studies and Community Targets for JWST's Early Release Science Program
Kevin B. Stevenson, Nikole K. Lewis, Jacob L. Bean +49
The James Webb Space Telescope will revolutionize transiting exoplanet atmospheric science due to its capability for continuous, long-duration observations and its larger collectin…
Quantifying and Predicting the Presence of Clouds in Exoplanet Atmospheres
Kevin B. Stevenson
One of the most outstanding issues in exoplanet characterization is understanding the prevalence of obscuring clouds and hazes in their atmospheres. The ability to predict the pres…