activity
20002022
most citedThe European Photon Imaging Camera on XMM-Newton: The MOS Cameras

2.4k citations · 2.9k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.IM2022★ 4 cited

Spectral performance of the Microchannel X-ray Telescope on board the SVOM mission

B. Schneider, N. Renault-Tinacci, D. Götz +7

The Microchannel X-ray Telescope (MXT) is an innovative compact X-ray instrument on board the SVOM astronomical mission dedicated to the study of transient phenomena such as gamma-…

astro-ph.IM2022★ 18 cited

The Scientific Performance of the Microchannel X-ray Telescope on board the SVOM Mission

D. Gotz, M. Boutelier, V. Burwitz +17

The Microchannel X-ray Telescope (MXT) will be the first focusing X-ray telescope based on a "Lobster-Eye" optical design to be flown on Sino-French mission SVOM. SVOM will be dedi…

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.HE2019★ 1 cited

PHEMTO : Polarimetric High Energy Modular Telescope Observatory

P. Laurent, F. Acero, V. Beckmann +27

With the opening of the X and gamma--ray windows in the sixties, thanks to to sounding rockets and satellite-borne instruments, extremely energetic and violent phenomena were disco…

astro-ph.IM2018★ 8 cited

The Athena X-ray Integral Field Unit

Didier Barret, Thien Lam Trong, Jan-Willem den Herder +100

The X-ray Integral Field Unit (X-IFU) is the high resolution X-ray spectrometer of the ESA Athena X-ray observatory. Over a field of view of 5' equivalent diameter, it will deliver…

astro-ph.IM2015★ 3 cited

Fine pitch CdTe-based Hard-X-ray polarimeter performance for space science in the 70-300 keV energy range

S. Antier, O. Limousin, P. Ferrando

X-rays astrophysical sources have been almost exclusively characterized through imaging, spectroscopy and timing analysis. Nevertheless, more observational parameters are needed be…