activity
19952012
most citedThe WARPS X-ray survey of galaxies, groups and clusters I: Method and first results

149 citations · 570 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.CO2012★ 11 cited

The WARPS Survey. VIII. Evolution of the Galaxy Cluster X-ray Luminosity Function

L. A. Koens, B. J. Maughan, L. R. Jones +5

We present measurements of the galaxy cluster X-ray Luminosity Function (XLF) from the Wide Angle ROSAT Pointed Survey (WARPS) and quantify its evolution. WARPS is a serendipitous…

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-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…

astro-ph2001★ 89 cited

The WARPS Survey: VI. Galaxy Cluster and Source Identifications from Phase I

E. S. Perlman, D. J. Horner, L. R. Jones +4

We present in catalog form the optical identifications for objects from the first phase of the Wide Angle ROSAT Pointed Survey (WARPS). WARPS is a serendipitous survey of relativel…

astro-ph2000★ 74 cited

Discovery of a very X-ray luminous galaxy cluster at z=0.89 in the WARPS survey

H. Ebeling, L. R. Jones, B. W. Fairley +3

We report the discovery of the galaxy cluster ClJ1226.9+3332 in the Wide Angle ROSAT Pointed Survey (WARPS). At z=0.888 and L_X=1.1e45 erg/s (0.5-2.0 keV, h_0=0.5) ClJ1226.9+3332 i…

astro-ph2000

The X-ray evolution of clusters of galaxies to z=0.9

L. R. Jones, H. Ebeling, C. Scharf +6

The evolution of the X-ray luminosity function of clusters of galaxies has been measured to z=0.9 using over 150 X-ray selected clusters discovered in the WARPS survey. We find no…