9C continued: a radio-source survey at 15 GHz (2009)
Waldram, E. M., Pooley, G. G., Davies, M. L., Grainge, K. J. B., Scott, P. F.
In our first paper we described three regions of the 9C survey of radio sources with the Ryle telescope at 15.2 GHz, constituting a total area of 520 deg^2 to a completeness limit of approximately 25...
An excess of emission in the dark cloud LDN 1111 with the Arcminute Microkelvin Imager (2008)
Hurley-Walker, N., Green, D. A., Davies, M. L., Grainge, K. J. B., Hobson, M. P., ...
We present observations of the Lynds' dark nebula LDN 1111 made at microwave frequencies between 14.6 and 17.2 GHz with the Arcminute Microkelvin Imager (AMI). We find emission in this frequency band...
Feroz, F., Hobson, M. P., Zwart, J. T. L., Saunders, R. D. E., Grainge, K. J. B.
We present a Bayesian approach to modelling galaxy clusters using multi-frequency pointed observations from telescopes that exploit the Sunyaev--Zel'dovich effect. We use the recently developed...
The Arcminute Microkelvin Imager (2008)
Barker, R. W., Biddulph, P., Bly, D., Boysen, R. C., Brown, A. R., ...
The Arcminute Microkelvin Imager is a pair of interferometer arrays operating with six frequency channels spanning 13.9-18.2 GHz, with very high sensitivity to angular scales 30''-10'. The telescope...
AMI limits on 15 GHz excess emission in northern HII regions (2007)
Scaife, A. M. M., Hurley-Walker, N., Davies, M. L., Duffett-Smith, P. J., Feroz, F., Grainge, K. J. B., ...
We present observations between 14.2 and 17.9 GHz of sixteen Galactic HII regions made with the Arcminute Microkelvin Imager (AMI). In conjunction with data from the literature at lower radio...
CLOVER: The CMB Polarization Observer (2005)
Maffei, B., Ade, P.A.R., Calderon, C., Challinor, A.D., De Bernardis, P., Dunlop, L., ...
We present a new, fully-funded ground-based instrument designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB). The concept is based on three independent sub-systems...
CLOVER Experiment: the receiver block (2005)
Pisano, G., Ade, P.A.R., Calderon, C., Challinor, A.D., De Bernardis, P., Dunlop, L., ...
The C$_{\it l}$OVER instrument (described elsewhere in this volume) is being built to measure the B-mode polarisation of the Cosmic Microwave Background. Each of the 256 pixels is made up a...
CLOVER: The CMB Polarization Observer (2005)
Maffei, B., Ade, P.A.R., Calderon, C., Challinor, A.D., De Bernardis, P., Dunlop, L., ...
We present a new, fully-funded ground-based instrument designed to measure the B-mode polarization of the Cosmic Microwave Background (CMB). The concept is based on three independent sub-systems...
CLOVER Experiment: the receiver block (2005)
Pisano, G., Ade, P.A.R., Calderon, C., Challinor, A.D., De Bernardis, P., Dunlop, L., ...
The C$_{\it l}$OVER instrument (described elsewhere in this volume) is being built to measure the B-mode polarisation of the Cosmic Microwave Background. Each of the 256 pixels is made up a...
Cosmology from Cluster SZ and Weak Lensing Data (2002)
Marshall, P. J., Lancaster, K., Hobson, M. P., Grainge, K. J. B.
Weak gravitational lensing and the Sunyaev-Zel'dovich effect provide complementary information on the composition of clusters of galaxies. Preliminary results from cluster SZ observations with the...