The origin of x-ray emission of two distant (z > 1) cluster candidates with XMM-Newton

Astronomy and Astrophysics

Volumn 406, Issue 3, 2003, Pages 789-795

  Neumann, D M ^a   Arnaud, M ^a   Benoist, C ^b   Da Costa, L ^c   Jorgensen H E ^d   Olsen, L F ^d   Bardelli, S ^e   Zucca, E ^e   Arnouts, S ^f   Biviano, A ^g   Ramella, M ^g  

^a CEA SACLAY   (France)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^d Astronomical Observatory ^*  (Denmark)

^e OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

^f AIX MARSEILLE UNIVERSITÉ   (France)

^g INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

Author keywords

Cosmology: large scale structure of universe; Cosmology: observations; EIS J0533 2412; Galaxies: active; Galaxies: clusters: individual: CL J0533 2411; X rays: galaxies: clusters

Indexed keywords

GALAXIES; INFRARED SPECTROSCOPY; SPACE RESEARCH; X RAYS;

CLUSTER EVOLUTION; COSMOLOGY;

ASTROPHYSICS;

EID: 0042698749     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030657     Document Type: Article

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