238 citations · 1.9k across the 78 of their papers we have counts for
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Signatures of Clouds in Hot Jupiter Atmospheres: Modeled High Resolution Emission Spectra from 3D General Circulation Models
Caleb K. Harada, Eliza M. -R. Kempton, Emily Rauscher +4
Observations of scattered light and thermal emission from hot Jupiter exoplanets have suggested the presence of inhomogeneous aerosols in their atmospheres. 3D general circulation…
The Precision of Mass Measurements Required for Robust Atmospheric Characterization of Transiting Exoplanets
Natasha E. Batalha, Taylor Lewis, Jonathan J. Fortney +4
Two of TESS's major science goals are to measure masses for 50 planets smaller than 4 Earth radii and to discover high-quality targets for atmospheric characterization efforts. It…
Simultaneous Optical Transmission Spectroscopy of a Terrestrial, Habitable-Zone Exoplanet with Two Ground-Based Multi-Object Spectrographs
Hannah Diamond-Lowe, Zachory Berta-Thompson, David Charbonneau +2
Investigating the atmospheres of rocky exoplanets is key to performing comparative planetology between these worlds and the terrestrial planets that reside in the inner solar syste…
Water Vapor and Clouds on the Habitable-Zone Sub-Neptune Exoplanet K2-18b
Björn Benneke, Ian Wong, Caroline Piaulet +13
Results from the Kepler mission indicate that the occurrence rate of small planets ( ) in the habitable zone of nearby low-mass stars may be as high as 80%. Despite t…
High-resolution Infrared Spectrograph for Exoplanet Characterization with the Keck and Thirty Meter Telescopes
Dimitri Mawet, Michael Fitzgerald, Quinn Konopacky +46
HISPEC (High-resolution Infrared Spectrograph for Exoplanet Characterization) is a proposed diffraction-limited spectrograph for the W.M. Keck Observatory, and a pathfinder for the…
Identifying Candidate Atmospheres on Rocky M dwarf Planets via Eclipse Photometry
Daniel D. B. Koll, Matej Malik, Megan Mansfield +4
Most rocky planets in the galaxy orbit a cool host star, and there is large uncertainty among theoretical models whether these planets can retain an atmosphere. The James Webb Spac…