The XMM-Newton Ω project I. The X-ray luminosity-temperature relation at z > 0.4

Astronomy and Astrophysics

Volumn 420, Issue 3, 2004, Pages 853-872

  Lumb, D H ^a   Bartlett, J G ^b,c   Romer, A K ^d,h   Blanchard, A ^e   Burke, D J ^f   Collins, C A ^g   Nichol, R C ^d   Giard, M ^e   Marty, P B ^e   Nevalainen, J ^f   Sadat, R ^e   Vauclair, S C ^e  

^a EUROPEAN SPACE AGENCY   (Netherlands)

^b UNIVERSITÉ PARIS DESCARTES   (France)

^c Lab de Physique Théorique   (France)

^d CARNEGIE MELLON UNIVERSITY   (United States)

^e IRAP   (France)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g LIVERPOOL JOHN MOORES UNIVERSITY   (United Kingdom)

^h UNIVERSITY OF SUSSEX   (United Kingdom)

Author keywords

Clusters; Galaxies; X rays

Indexed keywords

ASTROPHYSICS; COMPUTER SIMULATION; DATA REDUCTION; ESTIMATION; GALAXIES; MATHEMATICAL MODELS; ROBUSTNESS (CONTROL SYSTEMS); X RAY SPECTROSCOPY;

COSMOLOGY; EQUATION OF STATE; GALAXY: CLUSTERS; REDSHIFTS;

X RAYS;

EID: 3042636775     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035687     Document Type: Article

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