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Surveying the foreground sources for the Very Small Array, with the Ryle Telescope at 15 GHz

Published online by Cambridge University Press:  26 May 2016

E. M. Waldram  and
G. G. Pooley
E. M. Waldram
Affiliation:
Astrophysics Group, Cavendish Laboratory, Madingley Road, Cambridge, CB3 0HE, UK
G. G. Pooley
Affiliation:
Astrophysics Group, Cavendish Laboratory, Madingley Road, Cambridge, CB3 0HE, UK

Abstract

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The three fields chosen for the first observations with the Very Small Array (VSA), a total area of ˜ 200 deg2, are being surveyed with the Ryle Telescope at 15 GHz. This is the only wide-field survey at a comparable radio frequency; its purpose is to investigate the source population and to define a catalogue of the foreground sources which must be monitored by the VSA during its observations. We present preliminary source counts.

Type
Part XII: Poster Papers
Information
Symposium - International Astronomical Union , Volume 201: New Cosmological Data and the Values of the Fundamental Parameters , 2005 , pp. 525 - 526
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

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