Separating polarized cosmological and galactic emissions for cosmic microwave background B-mode polarization experiments

Monthly Notices of the Royal Astronomical Society

Volumn 372, Issue 2, 2006, Pages 615-629

  Stivoli, Federico ^a   Baccigalupi, Carlo ^a,b,c,d   Maino, Davide ^e   Stompor, Radek ^d,f,g  

^a SISSA   (Italy)

^b UNIVERSITY OF HEIDELBERG   (Germany)

^c SEZIONE DI TRIESTE   (Italy)

^d LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^e UNIVERSITY OF MILAN   (Italy)

^f UNIVERSITY OF CALIFORNIA   (United States)

^g UNIVERSITÉ PARIS DIDEROT   (France)

Author keywords

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

Indexed keywords

ANISOTROPY; GRAVITATIONAL EFFECTS; GRAVITY WAVES; IMAGE PROCESSING; INDEPENDENT COMPONENT ANALYSIS; INTELLIGENT SYSTEMS; MICROWAVES; MONTE CARLO METHODS; POLARIZATION; SEPARATION;

COMPONENT SEPARATION; COSMIC MICROWAVES BACKGROUND; COSMOLOGICAL MODELING; GALACTIC EMISSION; GHZ FREQUENCIES; INDEPENDENT COMPONENTS ANALYSIS; METHODS. DATA ANALYSIS; PARAMETER SPACES; SEPARATION TECHNIQUES; TECHNIQUES: IMAGE PROCESSING;

COSMOLOGY;

EID: 33749828330     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10769.x     Document Type: Article

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