activity
19952007
most citedScaling relations in fossil galaxy groups

126 citations · 261 across the 6 of their papers we have counts for

collaborators
Showing 2005Show all

6 papers · 1 filter

astro-ph2005

XMM observes ClJ0152.7-1357: A massive galaxy cluster forming at merger crossroads at z=0.83

B. J. Maughan, S. C. Ellis, L. R. Jones +3

We present an analysis of a 50ks XMM observation of the merging galaxy cluster ClJ0152.7-1357 at z=0.83. In addition to the two main subclusters and an infalling group detected in…

astro-ph2005

An analytic investigation of the scatter in the integrated X-ray properties of galaxy groups and clusters

Michael L. Balogh, Arif Babul, G. Mark Voit +4

(Abridged) We revisit the scaling relationships between the dark matter mass and observed X-ray luminosity and temperature of galaxy clusters and groups in the local Universe. Spec…

astro-ph2005

The XMM Large-Scale Structure Survey: An initial sample of galaxy groups and clusters to a redshift z<0.6

J. P. Willis, F. Pacaud, I. Valtchanov +14

We present X-ray and optical spectroscopic observations of twelve galaxy groups and clusters identified within the XMM Large-Scale Structure (LSS) survey. Groups and clusters are s…

astro-ph2005

The environmental dependence of galaxy colors in intermediate redshift X-ray-selected clusters

David A. Wake, Chris A. Collins, Robert C. Nichol +2

We present a wide-field imaging study of the colors of bright galaxies in 12 X-ray selected clusters and groups of galaxies at z ~ 0.3. The systems cover one of the largest ranges…

astro-ph2005

Batch discovery of nine z~1 clusters using x-ray and K or R,z' images

S. Andreon, I. Valtchanov, L. R. Jones +5

We present results of an initial search for clusters of galaxies at z~1 and above, using data from 2.9 square degrees of XMM-Newton images. By selecting weak potentially extended X…

astro-ph2005

The evolution of the cluster X-ray scaling relations in the WARPS sample at 0.6<z<1.0

B. J. Maughan, L. R. Jones, H. Ebeling +1

The X-ray properties of a sample of 11 high-redshift (0.6<z<1.0) clusters observed with Chandra and/or XMM are used to investigate the evolution of the cluster scaling relations. T…