246 citations · 2.1k across the 57 of their papers we have counts for
17 papers · 1 filter
A joint analysis of AMI and CARMA observations of the recently discovered SZ galaxy cluster system AMI-CL J0300+2613
AMI Consortium, :, Timothy W. Shimwell +16
We present CARMA observations of a massive galaxy cluster discovered in the AMI blind SZ survey. Without knowledge of the cluster redshift a Bayesian analysis of the AMI, CARMA and…
SZ observations with AMI of the hottest galaxy clusters detected in the XMM-Newton Cluster Survey
AMI Consortium, :, Timothy W. Shimwell +19
We have obtained deep SZ observations towards 15 of the apparently hottest XMM Cluster Survey (XCS) clusters that can be observed with the Arcminute Microkelvin Imager (AMI). We us…
AMI SZ observations and Bayesian analysis of a sample of six redshift-one clusters of galaxies
AMI Consortium, :, Michel P. Schammel +15
We present 16-GHz Sunyaev-Zel'dovich observations using the Arcminute Microkelvin Imager (AMI) and subsequent Bayesian analysis of six galaxy clusters at redshift () c…
Detailed SZ study of 19 LoCuSS galaxy clusters: masses and temperatures out to the virial radius
The AMI Consortium, :, Carmen Rodríguez-Gonzálvez +16
We present 16-GHz AMI SZ observations of 19 clusters with L_X >7x10^37 W (h50=1) selected from the LoCuS survey (0.142<z<0.295) and of A1758b, in the FoV of A1758a. We detect 17 cl…
Further Sunyaev-Zel'dovich observations of two Planck ERCSC clusters with the Arcminute Microkelvin Imager
The AMI Consortium, :, Natasha Hurley-Walker +17
We present follow-up observations of two galaxy clusters detected blindly via the Sunyaev-Zel'dovich (SZ) effect and released in the Planck Early Release Compact Source Catalogue.…
Sunyaev-Zel'dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: high X-ray luminosity sample
The AMI Consortium, :, Timothy W. Shimwell +16
We present observations from the Small Array of the Arcminute Microkelvin Imager (AMI) of eight high X-ray luminosity galaxy cluster systems selected from the Local Cluster Substru…
Bayesian analysis of weak gravitational lensing and Sunyaev-Zel'dovich data for six galaxy clusters
Natasha Hurley-Walker, Sarah Bridle, Eduardo S. Cypriano +19
We present an analysis of observations made with the Arcminute Microkelvin Imager (AMI) and the Canada-France-Hawaii Telescope (CFHT) of six galaxy clusters in a redshift range of…
Sunyaev-Zel'dovich observations of LoCuSS clusters with the Arcminute Microkelvin Imager: moderate X-ray luminosity sample
Carmen Rodriguez-Gonzalvez, Timothy W. Shimwell, Matthew L. Davies +14
We present 16-GHz observations using the Arcminute Microkelvin Imager (AMI) of 11 clusters with 7 x 10^{37}W < L_X < 11 x 10^{37}W (h_{50}=1.0) selected from the Local Cluster Subs…
Parameterization Effects in the analysis of AMI Sunyaev-Zel'dovich Observations
The AMI Consortium, :, Malak Olamaie +17
Most Sunyaev--Zel'dovich (SZ) and X-ray analyses of galaxy clusters try to constrain the cluster total mass and/or gas mass using parameterised models and assumptions of spherical…
10C Survey of Radio Sources at 15.7 GHz: I - Observing, mapping and source extraction
Thomas M. O. Franzen, Matthew L. Davies, Elizabeth M. Waldram +14
We have observed an area of approximatley 27 deg^2 to an rms noise level of less than 0.2 mJy at 15.7 GHz, using the Arcminute Microkelvin Imager Large Array. These observations co…
10C Survey of Radio Sources at 15.7 GHz: II - First Results
Matthew L. Davies, Thomas M. O. Franzen, Elizabeth M. Waldram +15
The first results from the Tenth Cambridge (10C) Survey of Radio Sources, carried out using the AMI Large Array (LA) at an observing frequency of 15.7 GHz, are presented. The surve…
Sunyaev-Zel'dovich observation of the Bullet-like cluster Abell 2146 with the Arcminute Microkelvin Imager
Carmen Rodriguez-Gonzalvez, Malak Olamaie, Matthew L. Davies +18
We present 13.9-18.2 GHz observations of the Sunyaev-Zel'dovich (SZ) effect towards Abell 2146 using the Arcminute Microkelvin Imager (AMI). The cluster is detected with a peak SNR…
Sunyaev-Zel'dovich observations of galaxy clusters out to the virial radius with the Arcminute Microkelvin Imager
Jonathan T. L. Zwart, Farhan Feroz, Matthew L. Davies +15
We present observations using the Small Array of the Arcminute Microkelvin Imager (AMI; 14-18 GHz) of four Abell and three MACS clusters spanning 0.171-0.686 in redshift. We detect…
Microwave observations of spinning dust emission in NGC6946
Anna M. M. Scaife, Bojan Nikolic, David A. Green +16
We report new cm-wave measurements at five frequencies between 15 and 18GHz of the continuum emission from the reportedly anomalous "region 4" of the nearby galaxy NGC6946. We find…
30 GHz observations of sources in the VSA fields
M. P. Gawronski, M. W. Peel, K. Lancaster +16
Small angular scale (high l) studies of cosmic microwave background anisotropies require accurate knowledge of the statistical properties of extragalactic sources at cm-mm waveleng…
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: II - Flux-density variability
Thomas M. O. Franzen, Matthew L. Davies, Rod D. Davies +22
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 Point Source…
Follow-up observations at 16 and 33 GHz of extragalactic sources from WMAP 3-year data: I - Spectral properties
Matthew L. Davies, Thomas M. O. Franzen, Rod D. Davies +22
We present follow-up observations of 97 point sources from the Wilkinson Microwave Anisotropy Probe (WMAP) 3-year data, contained within the New Extragalactic WMAP Point Source (NE…