activity
20072025
most citedCould we identify hot Ocean-Planets with CoRoT, Kepler and Doppler velocimetry?

103 citations · 111 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.IM2025

The X-ray Integral Field Unit at the end of the Athena reformulation phase

Philippe Peille, Didier Barret, Edoardo Cucchetti +279

The Athena mission entered a redefinition phase in July 2022, driven by the imperative to reduce the mission cost at completion for the European Space Agency below an acceptable ta…

astro-ph.IM2022★ 2 cited

The Athena X-ray Integral Field Unit: a consolidated design for the system requirement review of the preliminary definition phase

Didier Barret, Vincent Albouys, Jan-Willem den Herder +296

The Athena X-ray Integral Unit (X-IFU) is the high resolution X-ray spectrometer, studied since 2015 for flying in the mid-30s on the Athena space X-ray Observatory, a versatile ob…

astro-ph.IM2018

POLLUX: a UV spectropolarimeter for the LUVOIR space telescope project

Eduard Muslimov, Jean-Claude Bouret, Coralie Neiner +9

The present paper describes the current baseline optical design of POLLUX, a high-resolution spectropolarimeter for the future LUVOIR mission. The instrument will operate in the ul…

astro-ph2008★ 3 cited

Tests of achromatic phase shifters performed on the SYNAPSE test bench: a progress report

Pavel Gabor, Peter A. Schuller, Bruno Chazelas +16

The achromatic phase shifter (APS) is a component of the Bracewell nulling interferometer studied in preparation for future space missions (viz. Darwin/TPF-I) focusing on spectrosc…

astro-ph2008★ 3 cited

Stabilising a nulling interferometer using optical path difference dithering

Pavel Gabor, Bruno Chazelas, Frank Brachet +5

Context. Nulling interferometry has been suggested as the underlying principle for the Darwin and TPF-I exoplanet research missions. Aims. There are constraints both on the mean va…

astro-ph2007★ 103 cited

Could we identify hot Ocean-Planets with CoRoT, Kepler and Doppler velocimetry?

F. Selsis, B. Chazelas, P. Borde +16

Planets less massive than about 10 MEarth are expected to have no massive H-He atmosphere and a cometary composition (50% rocks, 50% water, by mass) provided they formed beyond the…