Cosmological implications of the maxima-1 high-resolution cosmic microwave background anisotropy measurement

Astrophysical Journal

Volumn 561, Issue 1 PART 2, 2001, Pages

  Stompor, R ^a,b,c   Abroe, M ^d   Ade, P ^e   Balbi, A ^f   Barbosa, D ^g,h   Bock, J ^i,j   Borrill, J ^g   Boscaleri, A ^k   De Bernardis, P ^l   Ferreira, P G ^m   Hanany, S ^d   Hristov, V ^j   Jaffe, A H ^a,b   Lee, A T ^a,g   Pascale, E ^k   Rabii, B ^a,b   Richards, P L ^a,b   Smoot, G F ^a,b,g   Winant, C D ^a,b   Wu, J H P ^a  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF CALIFORNIA   (United States)

^c NICOLAUS COPERNICUS ASTRONOMICAL CENTER   (Poland)

^d UNIVERSITY OF MINNESOTA   (United States)

^e QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^f UNIVERSITY OF ROME TOR VERGATA   (Italy)

^g LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^h INSTITUTO SUPERIOR TÉCNICO   (Portugal)

ⁱ CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^j CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^k CNR   (Italy)

^l UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

^m UNIVERSITY OF OXFORD   (United Kingdom)

more..

Author keywords

Cosmic microwave background; Cosmology: observations

Indexed keywords

EID: 0035511286     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324438     Document Type: Article

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