Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-yr data: II – Flux density variability

Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-yr data: II – Flux density variability

Using the Arcminute Microkelvin Imager (AMI) at 16 GHz and the Very Small Array (VSA)at 33 GHz to make follow-up observations of sources in the New Extragalactic WMAP PointSource catalogue, we have investigated the ?ux density variability in a complete sample of 97sources over time-scales of a few m...

Full description

Bibliographic Details
Main Authors: Franzen, Thomas, Davies, M., Davies, R., Davis, R., Feroz, F., Genova-Santos, R., Grainge, K., Green, D., Hobson, M., Hurley-Walker, Natasha, Lasenby, A., Lopez-Caniego, M., Olamaie, M., Padilla-Torres, C., Pooley, G., Rebolo, R., Rodriguez-Gonzalvez, C., Saunders, R., Scaife, A., Scott, P., Shimwell, T., Titterington, D., Waldram, E., Watson, R., Zwart, J.
Format: Journal Article
Published: Oxford University Press 2009
Subjects:
cosmic microwave background
- radio continuum: general
cosmology: observations
galaxies: active
Online Access:http://mnras.oxfordjournals.org/content/400/2/995.full.pdf+html
http://hdl.handle.net/20.500.11937/31998

Internet

http://mnras.oxfordjournals.org/content/400/2/995.full.pdf+html
http://hdl.handle.net/20.500.11937/31998

Similar Items