activity
20172021
most citedVUV-absorption cross section of carbon dioxide from 150 to 800 K and applications to warm exoplanetary atmospheres

53 citations · 80 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2021

Characterising atmospheric gravity waves on the nightside lower clouds of Venus: a systematic analysis

J. E. Silva, P. Machado, J. Peralta +3

We present the detection and characterisation of mesoscale waves on the lower clouds of Venus using images from the Visible Infrared Thermal Imaging Spectrometer onboard the Europe…

astro-ph.EP2021

3D convection-resolving model of temperate, tidally-locked exoplanets

Maxence Lefèvre, Martin Turbet, Raymond Pierrehumbert

A large fraction of known terrestrial-size exoplanets located in the Habitable Zone of M-dwarfs are expected to be tidally-locked. Numerous efforts have been conducted to study the…

astro-ph.IM202127 cited

Ariel: Enabling planetary science across light-years

Giovanna Tinetti, Paul Eccleston, Carole Haswell +313

Ariel, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, was adopted as the fourth medium-class mission in ESA's Cosmic Vision programme to be launched in 2029. Durin…

astro-ph.EP2021

TRAPPIST Habitable Atmosphere Intercomparison (THAI) workshop report

Thomas J. Fauchez, Martin Turbet, Denis E. Sergeev +31

The era of atmospheric characterization of terrestrial exoplanets is just around the corner. Modeling prior to observations is crucial in order to predict the observational challen…

astro-ph.EP2019

Mesoscale modeling of Venus' bow-shape waves

Maxence Lefèvre, Aymeric Spiga, Sébastien Lebonnois

The Akatsuki instrument LIR measured an unprecedented wave feature at the top of Venusian cloud layer. Stationary bow-shape waves of thousands of kilometers large lasting several E…

astro-ph.EP201753 cited

VUV-absorption cross section of carbon dioxide from 150 to 800 K and applications to warm exoplanetary atmospheres

Olivia Venot, Yves Bénilan, Nicolas Fray +9

Most exoplanets detected so far have atmospheric T significantly higher than 300K. Often close to their star, they receive an intense UV photons flux that triggers important photod…