WMAP 3-yr sources at 16 and 33GHz (Davies+, 2009)
Observations of the WMAP sources were made using the AMI-SA during 14 separate observing runs between 2007 April and 2008 September. Observations of the WMAP sources using VSA were performed during 10 separate observing runs between 2007 February and 2008 July. (1 data file).
Davies, M. L. et al.
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