Spider optimization: Probing the systematics of a large-scale B-mode experiment

Astrophysical Journal

Volumn 689, Issue 2, 2008, Pages 655-665

  Mactavish, C J ^a   Ade, P A R ^b   Battistelli, E S ^c   Benton, S ^d   Bihary, R ^e   Bock, J J ^f,g   Bond, J R ^a   Brevik, J ^f   Bryan, S ^e   Contaldi, C R ^h   Crill, B P ^a,d   Dore O ^a   Fissel, L ^d   Golwala, S R ^g   Halpern, M ^c   Hilton, G ⁱ   Holmes, W ^f   Hristov, V V ^g   Irwin, K ⁱ   Jones, W C ^f,g   Kuo, C L ^g   Lange, A E ^g   Lawrie, C ^e   Martin, T G ^d   Mason, P ^g   Montroy, T E ^e   Netterfield, C B ^d   Riley, D ^e   Ruhl, J E ^c   Runyan, M ^g   Trangsrud, A ^g   Tucker, C ^b   Turner, A ^f   Viero, M ^d   Wiebe, D ^d   more..

^a UNIVERSITY OF TORONTO   (Canada)

^b CARDIFF UNIVERSITY   (United Kingdom)

^c UNIVERSITY OF BRITISH COLUMBIA   (Canada)

^d UNIVERSITY OF TORONTO   (Canada)

^e CASE WESTERN RESERVE UNIVERSITY   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^h IMPERIAL COLLEGE LONDON   (United Kingdom)

ⁱ NATIONAL INSTITUTE OF STANDARDS AND TECHNOLOGY   (United States)

Author keywords

Cosmic microwave background; Gravitational waves methods: data analysis; Polarization

Indexed keywords

EID: 58149105600     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/592732     Document Type: Article

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