Astrophysical component separation of COBE-DMR 4-yr data with FASICA

Monthly Notices of the Royal Astronomical Society

Volumn 344, Issue 2, 2003, Pages 544-552

  Maino, D ^a   Banday, A J ^b   Baccigalupi, C ^c   Perrotta, F ^c   Gorski K M ^d,e,f  

^a UNIVERSITY OF MILAN   (Italy)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c SISSA   (Italy)

^d EUROPEAN SOUTHERN OBSERVATORY   (Germany)

^e UNIVERSITY OF WARSAW   (Poland)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Cosmic microwave background; Methods: Data analysis; Techniques: Image processing

Indexed keywords

DUST; IMAGE PROCESSING; INDEPENDENT COMPONENT ANALYSIS; RADIO ASTRONOMY; SIGNAL TO NOISE RATIO;

BACKGROUND SIGNALS; COMPONENT SEPARATION; COSMIC MICROWAVES BACKGROUND; COSMICS; DIFFERENTIAL MICROWAVE RADIOMETERS; FAST INDEPENDENT COMPONENT ANALYSIS; FREQUENCY-SCALING; GALACTIC EMISSION; METHODS. DATA ANALYSIS; TECHNIQUES: IMAGE PROCESSING;

COSMOLOGY;

EID: 0141886929     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06835.x     Document Type: Article

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