The X-ray properties of optically selected z > 0.6 clusters in the European Southern Observatory Distant Cluster Survey

Monthly Notices of the Royal Astronomical Society

Volumn 371, Issue 4, 2006, Pages 1777-1792

  Johnson, O ^a   Best, P ^a   Zaritsky, D ^b   Clowe, D ^b   Aragon Salamanca A ^c   Halliday, C ^d   Jablonka, P ^e   Milvang Jensen, B ^f   Pello R ^g   Poggianti, B M ^h   Rudnick, G ⁱ   Saglia, R ^j   Simard, L ^k   White, S ⁱ  

^a UK ASTRONOMY TECHNOLOGY CENTRE   (United Kingdom)

^b UNIVERSITY OF ARIZONA   (United States)

^c UNIVERSITY OF NOTTINGHAM   (United Kingdom)

^d INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^e OBSERVATOIRE DE PARIS   (France)

^f UNIVERSITY OF COPENHAGEN   (Denmark)

^g OBSERVATOIRE MIDI PYRÉNÉES   (France)

^h Oservatorio Astronomico   (Italy)

ⁱ MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^j MAX PLANCK INSTITUT FÜR EXTRATERRESTRISCHE PHYSIK   (Germany)

^k NATIONAL RESEARCH COUNCIL CANADA   (Canada)

more..

Author keywords

Galaxies: clusters: general; X rays: galaxies: clusters

Indexed keywords

COSMOLOGY; LUMINANCE; OBSERVATORIES; SPECTROSCOPIC ANALYSIS; SURVEYS;

CLUSTER SURVEY; EUROPEAN SOUTHERN OBSERVATORY; GALAXIES: CLUSTERS: GENERAL; HIGH-REDSHIFT; OPTICAL-; X-RAY LUMINOSITY; X-RAY PROPERTIES; X-RAY SURVEYS; X-RAYS GALAXIES CLUSTERS; XMM-NEWTON OBSERVATIONS;

GALAXIES;

EID: 33748683372     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10796.x     Document Type: Review

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