Protoclusters associated with z > 2 radio galaxies I. Characteristics of high redshift protoclusters

Astronomy and Astrophysics

Volumn 461, Issue 3, 2007, Pages 823-845

  Venemans, B P ^a,b   Rottgering H J A ^a   Miley, G K ^a   Van Breugel, W J M ^c,h   De Breuck, C ^d   Kurk, J D ^e   Pentericci, L ^f   Stanford, S A ^c,i   Overzier, R A ^a   Croft, S ^c,h   Ford, H ^g  

^a LEIDEN UNIVERSITY   (Netherlands)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^f INAF OSSERVATORIO ASTRONOMICO DI ROMA   (Italy)

^g JOHNS HOPKINS UNIVERSITY   (United States)

^h UNIVERSITY OF CALIFORNIA   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

Author keywords

Cosmology: early Universe; Cosmology: large scale structure of Universe; Cosmology: observations; Galaxies: active; Galaxies: clusters: general

Indexed keywords

COMPUTER SIMULATION; DISPERSION (WAVES); DOPPLER EFFECT; IMAGE ANALYSIS; IMAGE QUALITY; SPACE TELESCOPES;

COSMOLOGY; LARGE SCALE STRUCTURE; UNIVERSE; VELOCITY DISPERSION;

GALAXIES;

EID: 33846354531     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20053941     Document Type: Article

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