activity
20022011
most citedBlazars in the Fermi Era: The OVRO 40-m Telescope Monitoring Program

549 citations · 1.7k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2011★ 21 cited

Separating the BL Lac and Cluster X-ray Emissions in Abell 689 with Chandra

P. A. Giles, B. J. Maughan, M. Birkinshaw +2

We present the results of a Chandra observation of the galaxy cluster Abell 689 (z=0.279). Abell 689 is one of the most luminous clusters detected in the ROSAT All Sky Survey (RASS…

astro-ph.CO2011★ 13 cited

Sunyaev Zel'dovich observations of a statistically complete sample of galaxy clusters with OCRA-p

Katy Lancaster, Mark Birkinshaw, Marcin P. Gawronski +15

We present 30 GHz Sunyaev Zel'dovich observations of a statistically complete sample of galaxy clusters with OCRA-p. The clusters are the 18 most X-ray luminous clusters at z > 0.2…

astro-ph.CO2010★ 10 cited

A blind detection of a large, complex, Sunyaev--Zel'dovich structure

AMI Consortium, :, T. W. Shimwell +58

We present an interesting Sunyaev-Zel'dovich (SZ) detection in the first of the Arcminute Microkelvin Imager (AMI) 'blind', degree-square fields to have been observed down to our t…

astro-ph.CO2010★ 549 cited

Blazars in the Fermi Era: The OVRO 40-m Telescope Monitoring Program

Joseph L. Richards, Walter Max-Moerbeck, Vasiliki Pavlidou +20

The Large Area Telescope (LAT) aboard the Fermi Gamma-ray Space Telescope provides an unprecedented opportunity to study gamma-ray blazars. To capitalize on this opportunity, begin…

astro-ph.CO2010★ 8 cited

One Centimetre Receiver Array-prototype observations of the CRATES sources at 30 GHz

M. W. Peel, M. P. Gawronski, R. A. Battye +11

Knowledge of the population of radio sources in the range ~2-200 GHz is important for understanding their effects on measurements of the Cosmic Microwave Background power spectrum.…

astro-ph.GA2010★ 14 cited

A 33 GHz VSA survey of the Galactic plane from 27 to 46 degrees

M. Todorović, R. D. Davies, C. Dickinson +17

The Very Small Array (VSA) has been used to survey the l = 27 to 46 deg, |b|<4 deg region of the Galactic plane at a resolution of 13 arcmin. The survey consists of 44 pointings of…