A mature cluster with X-ray emission at z = 2.07

Astronomy and Astrophysics

Volumn 526, Issue 16, 2011, Pages

  Gobat, R ^a   Daddi, E ^a   Onodera, M ^b   Finoguenov, A ^c   Renzini, A ^d   Arimoto, N ^e,f   Bouwens, R ^g   Brusa, M ^c   Chary, R R ^h   Cimatti, A ⁱ   Dickinson, M ^j   Kong, X ^k   Mignoli, M ^l  

^a CEA SACLAY   (France)

^b ETH ZURICH   (Switzerland)

^c MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^d INAF OSSERVATORIO ASTRONOMICO DI PADOVA   (Italy)

^e NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^f GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

^g University of California at Santa Cruz   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF BOLOGNA   (Italy)

^j NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^k UNIVERSITY OF SCIENCE AND TECHNOLOGY OF CHINA   (China)

^l INAF OSSERVATORIO ASTRONOMICO DI BOLOGNA   (Italy)

more..

Author keywords

galaxies: clusters: general; galaxies: clusters: individual: CL J1449 0856; galaxies: high redshift; large scale structure of Universe

Indexed keywords

COMPACT CORES; EMISSION LINES; GALAXIES: CLUSTERS: GENERAL; GALAXIES: CLUSTERS: INDIVIDUAL: CL J1449-0856; GALAXIES: HIGH-REDSHIFT; GALAXY CLUSTERS; HALO MASS; LARGE SCALE STRUCTURE OF UNIVERSE; RED SHIFT; SPITZER; STELLAR MASS; X-RAY EMISSION; X-RAY LUMINOSITY; XMM-NEWTON;

ELECTROMAGNETIC WAVE EMISSION; ION BEAMS; LUMINANCE; X RAY SCATTERING; X RAYS;

GALAXIES;

EID: 78651289961     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201016084     Document Type: Article

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