activity
20122026
most citedGlobal modelling of the early Martian climate under a denser CO2 atmosphere: Water cycle and ice evolution

351 citations · 2.7k across the 54 of their papers we have counts for

collaborators
Showing 2020Show all

14 papers · 1 filter

astro-ph.EP202064 cited

A medium-resolution spectrum of the exoplanet HIP 65426 b

Simon Petrus, Mickaël Bonnefoy, Gaël Chauvin +18

Medium-resolution integral-field spectrographs (IFS) coupled with adaptive-optics such as Keck/OSIRIS, VLT/MUSE, or SINFONI are appearing as a new avenue for enhancing the detectio…

astro-ph.EP202084 cited

1D atmospheric study of the temperate sub-Neptune K2-18b

Doriann Blain, Benjamin Charnay, Bruno Bézard

The atmospheric composition of exoplanets with masses between 2 and 10 M is poorly understood. In that regard, the sub-Neptune K2-18b, which is subject to Earth-like stell…

astro-ph.EP202039 cited

ARES IV: Probing the atmospheres of the two warm small planets HD 106315 c and HD 3167 c with the HST/WFC3 camera

Gloria Guilluy, Amélie Gressier, Sam Wright +27

We present an atmospheric characterization study of two medium sized planets bracketing the radius of Neptune: HD 106315 c (R=4.98 0.23 R) and HD 3167 c…

astro-ph.EP202057 cited

Formation and dynamics of water clouds on temperate sub-Neptunes: The example of K2-18b

Benjamin Charnay, Doriann Blain, Bruno Bézard +3

Hubble (HST) spectroscopic transit observations of the temperate sub-Neptune K2-18b were interpreted as the presence of water vapour with potential water clouds. 1D modelling studi…

astro-ph.EP2020

Direct confirmation of the radial-velocity planet Pic c

M. Nowak, S. Lacour, A. -M. Lagrange +90

Methods used to detect giant exoplanets can be broadly divided into two categories: indirect and direct. Indirect methods are more sensitive to planets with a small orbital period,…

astro-ph.EP2020221 cited

Retrieving scattering clouds and disequilibrium chemistry in the atmosphere of HR 8799e

P. Mollière, T. Stolker, S. Lacour +25

Clouds are ubiquitous in exoplanet atmospheres and represent a challenge for the model interpretation of their spectra. Complex cloud models are too numerically costly for generati…