WMAP 3-yr sources at 16 and 33GHz. II. (Franzen+, 2009)
Using the Arcminute Microkelvin Imager (AMI) at 16GHz and the Very Small Array (VSA) at 33GHz to make follow-up observations of sources in the New Extragalactic WMAP Point Source catalogue, we have investigated the flux density variability in a complete sample of 97 sources over time-scales of a few months to ~1.5yr. (1 data file).
Franzen, T. M. O. et al.
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