activity
19972022
most citedThe Cosmic Lens All-Sky Survey: I. Source selection and observations

395 citations · 7.8k across the 118 of their papers we have counts for

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Showing 2004Show all

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astro-ph2004★ 219 cited

Polarization Observations with the Cosmic Background Imager

A. C. S. Readhead, S. T. Myers, T. J. Pearson +23

Polarization observations of the cosmic microwave background with the Cosmic Background Imager from September 2002 to May 2004 provide a significant detection of the E-mode polariz…

astro-ph2004★ 38 cited

CLASS B2108+213: A new wide separation gravitational lens system

J. P. McKean, I. W. A. Browne, N. J. Jackson +15

We present observations of CLASS B2108+213, the widest separation gravitational lens system discovered by the Cosmic Lens All-Sky Survey. Radio imaging using the VLA at 8.46 GHz an…

astro-ph2004★ 32 cited

An Unbiased Measurement of Ho through Cosmic Background Imager Observations of the Sunyaev-Zel'dovich Effect in Nearby Galaxy Clusters

P. S. Udomprasert, B. S. Mason, A. C. S. Readhead +1

We present Ho results from Cosmic Background Imager (CBI) observations of the Sunyaev-Zel'dovich Effect (SZE) in 7 galaxy clusters, A85, A399, A401, A478, A754, A1651, and A2597. T…

astro-ph2004★ 42 cited

The radio source population at high frequency: follow-up of the 15-GHz 9C survey

R. C. Bolton, G. Cotter, G. G. Pooley +6

We have carried out extensive radio and optical follow-up of 176 sources from the 15 GHz 9th Cambridge survey. Optical identifications have been found for 155 of the radio sources;…

astro-ph2004★ 17 cited

Vela X at 31 GHz

A. S. Hales, S. Casassus, H. Alvarez +6

We present observations of the Vela X region at 31 GHz using the Cosmic Background Imager (CBI). We find a strong compact radio source (5.9'x4.1', FWHM) about the Vela pulsar, whic…

astro-ph2004★ 329 cited

Extended Mosaic Observations with the Cosmic Background Imager

A. C. S. Readhead, B. S. Mason, C. R. Contaldi +18

Two years of microwave background observations with the Cosmic Background Imager (CBI) have been combined to give a sensitive, high resolution angular power spectrum over the range…