Sources in VSA fields at 30GHz (Gawronski+, 2010)

Details Sources in VSA fields at 30GHz (Gawronski+, 2010) Sources in VSA fields at 30GHz (Gawronski+, 2010)

Feb 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011ycat..74061853g&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/406/1853. Originally published in: 2010MNRAS.406.1853G

Computer Science

Radio Sources

Scientific paper

The VSA (Very Small Array) has made CMB observations in three different configurations, corresponding to different multipole order (l) ranges: compact for l=150-800 (Taylor et al. 2003, Cat. J/MNRAS/341/1066), extended for l=300-1500 (Dickinson et al. 2004MNRAS.353..732D) and super-extended for l=600-2500. The corresponding areas have been surveyed with the Ryle Telescope (RT) at 15GHz, to a greater depth the higher the l value, in order to identify the sources for subtraction at 33GHz. The five fields analyzed in this paper are those of the VSA super-extended observations.
(2 data files).

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