Very Small Array. Flux density at 33GHz (Cleary+, 2005)
We describe the source subtraction strategy and observations for the extended Very Small Array (VSA), a cosmic microwave background interferometer operating at...
Very Small Array. Flux density at 33GHz (Cleary+, 2005)
We describe the source subtraction strategy and observations for the extended Very Small Array (VSA), a cosmic microwave background interferometer operating at...
Very Small Array. II. CMB at 34GHz (Taylor+, 2003)
We have observed the cosmic microwave background (CMB) temperature fluctuations in eight fields covering three separated areas of sky with the Very Small Array...
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...
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...