Multi-wavelength study of XMMU J2235.3-2557: The most massive galaxy cluster at z >1

Astronomy and Astrophysics

Volumn 508, Issue 2, 2009, Pages 583-591

  Rosati, P ^a   Tozzi, P ^b,m   Gobat, R ^c   Santos, J S ^b   Nonino, M ^b   Demarco, R ^e   Lidman, C ^d,n   Mullis, C R ^g   Strazzullo, V ^f   Bohringer H ⁱ   Fassbender, R ⁱ   Dawson, K ^h   Tanaka, M ^a   Jee, J ^l   Ford, H ^k   Lamer, G ^j   Schwope, A ^j  

^a EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^b INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^c CEA SACLAY   (France)

^d EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^e UNIVERSITY OF CONCEPCIÓN   (Chile)

^f NATIONAL RADIO ASTRONOMY OBSERVATORY   (United States)

^g Wachovia Corp   (United States)

^h UNIVERSITY OF UTAH   (United States)

ⁱ MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^j ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^k JOHNS HOPKINS UNIVERSITY   (United States)

^l UNIVERSITY OF CALIFORNIA   (United States)

^m SEZIONE DI TRIESTE   (Italy)

ⁿ STOCKHOLM UNIVERSITY   (Sweden)

more..

Author keywords

Galaxies: clusters: individual: XMMU J2235.3 2557; Galaxies: evolution; Galaxies: high redshift X rays: galaxies: clusters

Indexed keywords

CHANDRA; EVOLUTIONARY STAGE; GALAXIES: CLUSTERS: INDIVIDUALS; GALAXIES: EVOLUTIONS; GALAXY CLUSTERS; HOT GAS; HYDROSTATIC EQUILIBRIUM; IMAGING DATA; INTRA-CLUSTER; MEAN AGES; METAL ABUNDANCES; METALLICITIES; MULTI-WAVELENGTH STUDY; MULTIWAVELENGTH; RADIAL GRADIENT; RED SHIFT; SPECTRAL ENERGY DISTRIBUTION; SPECTRAL SIGNATURE; SPECTRAL SYNTHESIS; SPECTROSCOPIC DATA; STAR FORMATIONS; STELLAR MASS; SURFACE BRIGHTNESS; THERMODYNAMICAL PROPERTIES; TOTAL MASS; X RAYS: GALAXIES: CLUSTERS; X-RAY TEMPERATURES;

ASTROPHYSICS; HARMONIC ANALYSIS; POPULATION STATISTICS; SPECTROSCOPY; SPECTRUM ANALYSIS; STARS; X RAYS;

GALAXIES;

EID: 77951842365     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913099     Document Type: Article

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