activity
20072021
most citedThe XMM-LSS survey: the Class 1 cluster sample over the initial 5 square degrees and its cosmological modelling

172 citations · 678 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.CO2021★ 36 cited

The XXL survey: XLVI. Forward cosmological analysis of the C1 cluster sample

Christian Garrel, Marguerite Pierre, Patrick Valageas +15

We present the forward cosmological analysis of an selected sample of galaxy clusters out to a redshift of unity. Following our previous 2018 study based on the dn/dz quantit…

astro-ph.CO2015★ 143 cited

The XXL Survey. II. The bright cluster sample: catalogue and luminosity function

F. Pacaud, N. Clerc, P. A. Giles +40

Context. The XXL Survey is the largest survey carried out by the XMM-Newton satellite and covers a total area of 50 square degrees distributed over two fields. It primarily aims at…

astro-ph.CO2015★ 89 cited

The XXL Survey IV. Mass-temperature relation of the bright cluster sample

Maggie Lieu, Graham P. Smith, Paul A. Giles +18

The XXL survey is the largest survey carried out by XMM-Newton. Covering an area of 50deg, the survey contains galaxy clusters out to a redshift 2 and to an X-r…

astro-ph.CO2014★ 32 cited

The X-CLASS - redMaPPer galaxy cluster comparison: I. Identification procedures

Tatyana Sadibekova, Marguerite Pierre, Nicolas Clerc +5

We performed a detailed and, for a large part interactive, analysis of the matching output between the X-CLASS and redMaPPer cluster catalogues. The overlap between the two catalog…

astro-ph.CO2011★ 72 cited

The cosmological analysis of X-ray cluster surveys: II- Application of the CR-HR method to the XMM archive

Nicolas Clerc, Tatyana Sadibekova, Marguerite Pierre +5

We have processed 2774 high-galactic observations from the XMM archive (as of May 2010) and extracted a serendipitous catalogue of some 850 clusters of galaxies based on purely X-r…

astro-ph.CO2010★ 64 cited

The XMM-LSS survey: optical assessment and properties of different X-ray selected cluster classes

C. Adami, A. Mazure, M. Pierre +29

XMM and Chandra opened a new area for the study of clusters of galaxies. Not only for cluster physics but also, for the detection of faint and distant clusters that were inaccessib…

astro-ph2007★ 172 cited

The XMM-LSS survey: the Class 1 cluster sample over the initial 5 square degrees and its cosmological modelling

F. Pacaud, M. Pierre, C. Adami +30

We present a sample of 29 galaxy clusters from the XMM-LSS survey over an area of some 5deg2 out to a redshift of z=1.05. The sample clusters, which represent about half of the X-r…

astro-ph2007★ 70 cited

The XMM-LSS catalogue: X-ray sources and associated optical data. Version I

M. Pierre, L. Chiappetti, F. Pacaud +34

Following the presentation of the XMM-LSS X-ray source detection package by Pacaud et al., we provide the source lists for the first 5.5 surveyed square degrees. The catalogues per…