Galactic foreground constraints from the Python V cosmic microwave background anisotropy data

Astrophysical Journal

Volumn 592, Issue 2 I, 2003, Pages 692-698

  Mukherjee, Pia ^a,b   Coble, Kim ^c,d   Dragovan, Mark ^e   Ganga, Ken ^f   Kovac, John ^c   Ratra, Bharat ^a   Souradeep, Tarun ^a,g  

^a KANSAS STATE UNIVERSITY   (United States)

^b University of Oklahoma   (United States)

^c UNIVERSITY OF CHICAGO   (United States)

^d ADLER PLANETARIUM   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g INTER UNIVERSITY CENTRE FOR ASTRONOMY AND ASTROPHYSICS   (India)

Author keywords

Cosmic microwave background; Cosmology: observations; Diffuse radiation; Dust, extinction

Indexed keywords

EID: 0042917973     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/375860     Document Type: Article

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