Angular power spectrum of the fastica cosmic microwave background component from Background Emission Anisotropy Scanning Telescope data

Monthly Notices of the Royal Astronomical Society

Volumn 369, Issue 1, 2006, Pages 441-448

  Donzelli, S ^a,b   Maino, D ^a   Bersanelli, M ^a   Childers, J ^c   Figueiredo, N ^d   Lubin, P M ^c   Meinhold, P R ^c   O'Dwyer, I J ^e   Seiffert, M D ^f   Villela, T ^g   Wandelt, B D ^e   Wuensche, C A ^g  

^a UNIVERSITY OF MILAN   (Italy)

^b SISSA   (Italy)

^c UNIVERSITY OF CALIFORNIA   (United States)

^d FEDERAL UNIVERSITY OF ITAJUBÁ   (Brazil)

^e UNIVERSITY OF ILLINOIS AT URBANA CHAMPAIGN   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g INSTITUTO NACIONAL DE PESQUISAS ESPACIAIS   (Brazil)

Author keywords

Cosmic microwave background; Methods: data analysis; Techniques: image processing

Indexed keywords

ANISOTROPY; COSMIC RAYS; IMAGE PROCESSING; MICROWAVES; MONTE CARLO METHODS; POWER SPECTRUM; TELESCOPES;

ANGULAR POWER SPECTRUM; BACKGROUND COMPONENTS; BACKGROUND EMISSIONS; COSMIC MICROWAVES BACKGROUND; EMISSION ANISOTROPY; FAST-ICA; FASTICA; METHODS. DATA ANALYSIS; TECHNIQUES: IMAGE PROCESSING; TELESCOPE DATA;

COSMOLOGY;

EID: 33745256997     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10320.x     Document Type: Article

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