No CrossRef data available.
Article contents
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
Abstract
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
- Copyright
- Copyright © Astronomical Society of the Pacific 2005