Testing the galaxy cluster mass-observable relations at z = 1 with XMM-Newton and Chandra observations of XLSSJ022403.9-041328

Monthly Notices of the Royal Astronomical Society

Volumn 387, Issue 3, 2008, Pages 998-1006

  Maughan, B J ^a,b   Jones, L R ^c   Pierre, M ^d   Andreon, S ^e   Birkinshaw, M ^b   Bremer, M N ^b   Pacaud, F ^f   Ponman, T J ^c   Valtchanov, I ^g   Willis, J ^h  

^a UNIVERSITY OF BRISTOL   (United Kingdom)

^b HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^c UNIVERSITY OF BIRMINGHAM   (United Kingdom)

^d UNIVERSITÉ PARIS DIDEROT   (France)

^e INAF IASF MILANO   (Italy)

^f UNIVERSITY OF BONN   (Germany)

^g EUROPEAN SPACE AGENCY   (Spain)

^h UNIVERSITY OF VICTORIA   (Canada)

Author keywords

Cosmology: observations; Galaxies: clusters: general; Galaxies: high redshift; Intergalactic medium; X rays: galaxies

Indexed keywords

GALAXIES;

CHANDRA; COSMOLOGY OBSERVATIONS; GALAXIES CLUSTERS; GALAXIES: CLUSTERS: GENERAL; GALAXIES:HIGH-REDSHIFT; INTERGALACTIC MEDIUM; MASS-FRACTION; SCALING RELATIONS; X-RAYS: GALAXIES; XMM-NEWTON;

COSMOLOGY;

EID: 45249090352     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13313.x     Document Type: Article

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