activity
19992025
most citedThe Herschel-SPIRE instrument and its in-flight performance

2.2k citations · 2.5k across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2025★ 12 cited

MIRI-LRS spectrum of a cold exoplanet around a white dwarf: water, ammonia, and methane measurements

Maël Voyer, Quentin Changeat, Pierre-Olivier Lagage +21

The study of the atmosphere of exoplanets orbiting white dwarfs is a largely unexplored field. With WD\,0806-661\,b, we present the first deep dive into the atmospheric physics and…

astro-ph.CO2016★ 12 cited

The cosmological analysis of X-ray cluster surveys; III. 4D X-ray observable diagrams

M. Pierre, A. Valotti, L. Faccioli +4

Despite compelling theoretical arguments, the use of clusters as cosmological probes is, in practice, frequently questioned because of the many uncertainties impinging on cluster m…

astro-ph.IM2010★ 2.2k cited

The Herschel-SPIRE instrument and its in-flight performance

M. J. Griffin, A. Abergel, A. Abreu +176

The Spectral and Photometric Imaging Receiver (SPIRE), is the Herschel Space Observatory`s submillimetre camera and spectrometer. It contains a three-band imaging photometer operat…

astro-ph.GA2010★ 60 cited

The Herschel view of star formation in the Rosette molecular cloud under the influence of NGC 2244

N. Schneider, F. Motte, S. Bontemps +43

The Rosette molecular cloud is promoted as the archetype of a triggered star-formation site. This is mainly due to its morphology, because the central OB cluster NGC 2244 has blown…

astro-ph2000★ 166 cited

Measuring Cluster Temperature Profiles with XMM/EPIC

M. Arnaud, D. M. Neumann, N. Aghanim +3

Using the PV observation of A1795, we illustrate the capability of XMM-EPIC to measure cluster temperature profiles, a key ingredient for the determination of cluster mass profiles…

astro-ph1999★ 1 cited

An XMM pre-view of the cosmic network: galaxy groups and filaments

M. Pierre, G. Bryan, R. Gastaud

A large fraction of the baryons today are predicted to be in hot, filamentary gas, which has yet to be detected. In this paper, we use numerical simulations of dark matter and gas…