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

C Adami; A Mazure; M Pierre; PG Sprimont; C Libbrecht; F Pacaud; N Clerc; Trevor Ponman

doi:10.1051/0004-6361/201015182

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

C Adami, A Mazure, M Pierre, PG Sprimont, C Libbrecht, F Pacaud, N Clerc, Trevor Ponman

Physics and Astronomy

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8 Citations (Scopus)

Abstract

Context. 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 inaccessible with previous missions. Aims. This article presents 66 spectroscopically confirmed clusters (0.05

Original language	English
Article number	A18
Pages (from-to)	A18
Journal	Astronomy and Astrophysics
Volume	526
DOIs	https://doi.org/10.1051/0004-6361/201015182
Publication status	Published - 1 Feb 2011

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10.1051/0004-6361/201015182

Birmingham Astrophysics - Rolling Grant 2007-2012
Ponman, T. (Principal Investigator), Cruise, M. (Co-Investigator), Freise, A. (Co-Investigator), Raychaudhury, S. (Co-Investigator), Smith, G. (Co-Investigator), Speake, C. (Co-Investigator), Stevens, I. (Co-Investigator) & Vecchio, A. (Co-Investigator)
SCIENCE & TECHNOLOGY FACILITIES COUNCIL
1/04/07 → 31/03/12
Project: Research Councils

Cite this

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

abstract = "Context. 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 inaccessible with previous missions. Aims. This article presents 66 spectroscopically confirmed clusters (0.05 ",

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AU - Adami, C

AU - Mazure, A

AU - Pierre, M

AU - Sprimont, PG

AU - Libbrecht, C

AU - Pacaud, F

AU - Clerc, N

AU - Ponman, Trevor

PY - 2011/2/1

Y1 - 2011/2/1

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AB - Context. 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 inaccessible with previous missions. Aims. This article presents 66 spectroscopically confirmed clusters (0.05

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DO - 10.1051/0004-6361/201015182

M3 - Article

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VL - 526

SP - A18

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

M1 - A18

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

Abstract

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Projects

Birmingham Astrophysics - Rolling Grant 2007-2012

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