Constraining the power spectrum using clusters

New Astronomy

Volumn 1, Issue 4, 1997, Pages 321-347

  Borgani, S ^a,b   Moscardini, L ^c   Plionis, M ^b,d   Gorski K M ^e,j   Holtzman, J ^f   Klypin, A ^f   Primack, J R ^g   Smith, C C ^f   Stompor, R ^h,i  

^a INFN SEZIONE DI PERUGIA   (Italy)

^b SISSA   (Italy)

^c UNIVERSITY OF PADOVA   (Italy)

^d NATIONAL OBSERVATORY OF ATHENS   (Greece)

^e HUGHES STX CORPORATION   (United States)

^f NEW MEXICO STATE UNIVERSITY   (United States)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h UNIVERSITY OF OXFORD   (United Kingdom)

ⁱ NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^j UNIVERSITY OF WARSAW   (Poland)

more..

Author keywords

Dark matter; Galaxies: clusters; Large scale structure of universe

Indexed keywords

EID: 0001066023     PISSN: 13841076     EISSN: None     Source Type: Journal    
DOI: 10.1016/S1384-1076(96)00021-8     Document Type: Article

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