We have observed the cosmic microwave background (CMB) temperature fluctuations in eight fields covering three separated areas of sky with the Very Small Array at 34GHz. A total area of 101 square degrees has been imaged, with sensitivity on angular scales of 3.6{deg}-0.4{deg} (equivalent to angular multipoles l=150-900).
Cone search capability for table J/MNRAS/341/1066/table1 (VSA field positions and total effective integration time remaining after flagging and filtering of the data)
Cone search capability for table J/MNRAS/341/1066/table3 (Point sources subtracted from VSA fields.)