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20182026
most citedThermal emission from the Earth-sized exoplanet TRAPPIST-1 b using JWST

239 citations · 2.5k across the 83 of their papers we have counts for

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Showing 2023Show all

15 papers · 1 filter

astro-ph.EP2023

Physical properties of Centaur (60558) 174P/Echeclus from stellar occultations

C. L. Pereira, F. Braga-Ribas, B. Sicardy +42

The Centaur (60558) Echeclus was discovered on March 03, 2000, orbiting between the orbits of Jupiter and Uranus. After exhibiting frequent outbursts, it also received a comet desi…

astro-ph.EP2023★ 128 cited

SO2, silicate clouds, but no CH4 detected in a warm Neptune

Achrene Dyrek, Michiel Min, Leen Decin +44

WASP-107b is a warm (~740 K) transiting planet with a Neptune-like mass of ~30.5 Earth masses and Jupiter-like radius of ~0.94 Jupiter radius, whose extended atmosphere is eroding.…

astro-ph.EP2023★ 36 cited

A roadmap for the atmospheric characterization of terrestrial exoplanets with JWST

TRAPPIST-1 JWST Community Initiative, :, Julien de Wit +80

Ultra-cool dwarf stars are abundant, long-lived, and uniquely suited to enable the atmospheric study of transiting terrestrial companions with JWST. Amongst them, the most prominen…

astro-ph.EP2023★ 37 cited

Water Condensation Zones around Main Sequence Stars

Martin Turbet, Thomas J. Fauchez, Jeremy Leconte +10

Understanding the set of conditions that allow rocky planets to have liquid water on their surface -- in the form of lakes, seas or oceans -- is a major scientific step to determin…

astro-ph.EP2023★ 3 cited

Potential Atmospheric Compositions of TRAPPIST-1 c constrained by JWST/MIRI Observations at 15 m

Andrew P. Lincowski, Victoria S. Meadows, Sebastian Zieba +13

The first JWST observations of TRAPPIST-1 c showed a secondary eclipse depth of 421+/-94 ppm at 15 um, which is consistent with a bare rock surface or a thin, O2-dominated, low CO2…

astro-ph.EP2023★ 27 cited

An M dwarf accompanied by a close-in giant orbiter with SPECULOOS

Amaury H. M. J. Triaud, Georgina Dransfield, Taiki Kagetani +40

In the last decade, a dozen close-in giant planets have been discovered orbiting stars with spectral types ranging from M0 to M4, a mystery since known formation pathways do not pr…