Multiple peaks in the angular power spectrum of the cosmic microwave background: Significance and consequences for cosmology

Astrophysical Journal

Volumn 564, Issue 2 I, 2002, Pages 559-566

  De Bernardis, P ^a   Ade, P A R ^b   Bock, J J ^c   Bond, J R ^d   Borrill, J ^e   Boscaleri, A ^f   Coble, K ^g   Contaldi, C R ^d   Crill, B P ^h   De Troia, G ^a   Farese, P ^g   Ganga, K ^h   Giacometti, M ^a   Hivon, E ^h   Hristov, V V ^h   Iacoangeli, A ^a   Jaffe, A H ⁱ   Jones, W C ^h   Lange, A E ^h   Martinis, L ^j   Masi, S ^a   Mason, P ^h   Mauskopf, P D ^k   Melchiorri, A ^l   Montroy, T ^g   Netterfield, C B ^m   Pascale, E ^f   Piacentini, F ^a   Pogosyan, D ^d   Polenta, G ^a   Pongetti, F ⁿ   Prunet, S ^d   Romeo, G ⁿ   Ruhl, J E ^g   Scaramuzzi, F ^j   more..

^a UNIVERSITÀ DI ROMA LA SAPIENZA   (Italy)

^b QUEEN MARY UNIVERSITY OF LONDON   (United Kingdom)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d UNIVERSITY OF TORONTO   (Canada)

^e LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^f CNR   (Italy)

^g UNIVERSITY OF CALIFORNIA   (United States)

^h CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

ⁱ UNIVERSITY OF CALIFORNIA   (United States)

^j ENEA   (Italy)

^k CARDIFF UNIVERSITY   (United Kingdom)

^l UNIVERSITY OF OXFORD   (United Kingdom)

^m UNIVERSITY OF TORONTO   (Canada)

ⁿ ISTITUTO NAZIONALE DI GEOFISICA E VULCANOLOGIA   (Italy)

more..

Author keywords

Cosmic microwave background; Cosmological parameters; Cosmology: observations

Indexed keywords

EID: 0000693914     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/324298     Document Type: Article

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