Do Temperate Rocky Planets Around M Dwarfs have an Atmosphere ?
DOYON R.
proceedings of the Pontifical Academy of Science workshop on The James Webb Space Telescope: from first light to new worldviews, Vatican City, 27-29 February 2024
, accepted
arxiv
LHS 1140 b is a potentially habitable water world
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ApJ. Letters
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paperarxiv
A reanalysis of the LHS 1140 b atmosphere observed with the Hubble Space Telescope
BIAGINI A., CRACCHIOLO G., PATRALIA A., MALDONADO J., DI MAIO C. & MICELA G.
MNRAS
, 530
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paperarxiv
Modeling the astrosphere of LHS~1140
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Astron. & Astrophys.
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arxiv
Probing Cold-to-Temperate Exoplanetary Atmospheres: The Role of Water Condensation on Surface Identification with JWST
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ApJ
, 975
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paperarxiv
New Mass and Radius Constraints on the LHS 1140 Planets -- LHS 1140 b is Either a Temperate Mini-Neptune or a Water World
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ApJ. Letters
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paperarxiv
Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST/NIRISS
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ApJ Letters
, 970
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paperarxiv
Potential Interior Structures and Habitability of Super-Earth Exoplanets LHS 1140 b, K2-18 b, TOI-1452 b and TOI-1468 c
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ApJ
, accepted
arxiv
Prospects for Cryovolcanic Activity on Cold Ocean Planets
QUICK L., ROBERGE A., MENDOZA G., QUINTANA R. & YOUNG BLOOD A.
ApJ
, 956
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Planetary Parameters, XUV Environments, and Mass-loss Rates for Nearby Gaseous Planets with X-Ray-detected Host Stars
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The Effects of Stellar Gravity Darkening on High-resolution Transmission Spectra
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Atmospheres of Rocky Exoplanets
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On The Hydrosphere Stability of TESS Targets: Applications to 700 d, 256 b, and 203 b
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Hubble WFC3 Spectroscopy of the Habitable-zone Super-Earth LHS 1140 b
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Exploring the Nature of a Temperate Exoplanet in the Fulton Gap