activity
20162024
most citedThe habitability of Proxima Centauri b II. Possible climates and Observability

263 citations · 562 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.IM20242 cited

ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developments

A. Marconi, M. Abreu, V. Adibekyan +286

The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion E…

astro-ph.IM2024

RISTRETTO: Manufacturing of a single-mode visible high resolution spectrograph

Bruno Chazelas, Christophe Lovis, Nicolas Blind +13

The Spectrograph of the RISTRETTO instrument is now currently being manufactured. RISTETTO is an instrument designed to detect and characterize the reflected light of nearby exopla…

astro-ph.EP20242 cited

Transmission Spectroscopy of the Habitable Zone Exoplanet LHS 1140 b with JWST/NIRISS

Charles Cadieux, René Doyon, Ryan J. MacDonald +20

LHS 1140 b is the second-closest temperate transiting planet to the Earth with an equilibrium temperature low enough to support surface liquid water. At 1.7300.025 R,…

astro-ph.EP20234 cited

3D Global climate model of an exo-Venus: a modern Venus-like atmosphere for the nearby super-Earth LP 890-9 c

Diogo Quirino, Gabriella Gilli, Lisa Kaltenegger +6

The recently discovered super-Earth LP 890-9 c is an intriguing target for atmospheric studies as it transits a nearby, low-activity late-type M-dwarf star at the inner edge of the…

astro-ph.EP202337 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

ATMOSPHERIX: II- Characterising exoplanet atmospheres through transmission spectroscopy with SPIRou

F. Debras, B. Klein, J. -F. Donati +26

In a companion paper, we introduced a publicly-available pipeline to characterise exoplanet atmospheres through high-resolution spectroscopy. In this paper, we use this pipeline to…