activity
19952009
most citedCombining Strong and Weak Gravitational Lensing in Abell 1689

304 citations · 1.5k across the 13 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

7 papers · 2 filters

astro-ph2003

A unique small-scale gravitational arc in Abell 1201

Alastair C. Edge, Graham P. Smith, David J. Sand +4

We present a snapshot Hubble Space Telescope (HST) image of the galaxy cluster A1201 (z=0.169), revealing a tangential arc 2arcsec from the brightest cluster galaxy (BCG). Keck-ESI…

astro-ph2003

Measuring the matter distribution within z=0.2 cluster lenses with XMM-Newton

P. B. Marty, J. -P. Kneib, R. Sadat +4

We present an analysis of 7 clusters observed by XMM as part of our survey of 17 most X-ray luminous clusters of galaxies at z=0.2 selected for a comprehensive and unbiased study o…

astro-ph20031 cited

Clusters in the Zone of Avoidance

D. D. Kocevski, H. Ebeling, C. R. Mullis

The Clusters in the Zone of Avoidance (CIZA) project is producing the first statistically complete catalogue of X-ray selected galaxy clusters behind the Galactic plane. Current op…

astro-ph2003

An XMM and Chandra view of massive clusters of galaxies to z=1

L. R. Jones, B. J. Maughan, H. Ebeling +7

The X-ray properties of a sample of high redshift (z>0.6), massive clusters observed with XMM-Newton and Chandra are described, including two exceptional systems. One, at z=0.89, h…

astro-ph200310 cited

Discovery of an overdensity of faint red galaxies in the vicinity of the z=1.786 radio galaxy 3C 294

S. Toft, K. Pedersen, H. Ebeling +1

We report the discovery of an overdensity of faint red galaxies in the vicinity of the z=1.786 radio galaxy 3C 294. The overdensity, discovered in a 84 min Ks-band ISAAC/VLT image…

astro-ph2003

The Evolution of Cluster Radio Galaxies at 0.5<z<1

Eric S. Perlman, Christopher Frye, Harald Ebeling +3

We are conducting a deep radio survey of a sample of 25 distant () clusters of galaxies. Here we present a progress report. So far 17 of 25 clusters have been observed, to…