Source subtraction for the extended Very Small Array and 33-GHz source count estimates

Monthly Notices of the Royal Astronomical Society

Volumn 360, Issue 1, 2005, Pages 340-353

  Cleary, Kieran A ^a,d   Taylor, Angela C ^b,e   Waldram, Elizabeth ^b   Battye, Richard A ^a   Dickinson, Clive ^a,f   Davies, Rod D ^a   Davis, Richard J ^a   Genova Santos, Ricardo ^c   Grainge, Keith ^b   Jones, Michael E ^b,e   Kneissl, Rüdiger ^b   Pooley, G G ^b   Rafael Rebolo, José ^c   Rubiño Martín, Alberto ^c   Saunders, Richard D E ^b   Scott, Paul F ^b   Slosar, Anže ^b,g   Titterington, David ^b   Watson, Robert A ^a,c  

^a UNIVERSITY OF MANCHESTER   (United Kingdom)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e UNIVERSITY OF OXFORD   (United Kingdom)

^f CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^g UNIVERSITY OF LJUBLJANA   (Slovenia)

Author keywords

Cosmic microwave background; Radio continuum: galaxies; Surveys

Indexed keywords

COSMIC MICROWAVES BACKGROUND; DENSITY RANGE; FLUX DENSITIES; POWER-SPECTRA; RADIO CONTINUUM: GALAXIES; SPECTRA'S;

COSMOLOGY;

EID: 20744441839     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09037.x     Document Type: Article

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