activity
19962009
most citedThe ROSAT-ESO Flux Limited X-ray (REFLEX) Galaxy Cluster Survey. V. The cluster catalogue

653 citations · 2.1k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.CO2009★ 61 cited

The REFLEX galaxy cluster survey. VIII. Spectroscopic observations and optical atlas

L. Guzzo, P. Schuecker, H. Boehringer +8

We present the final data from the spectroscopic survey of the ROSAT-ESO Flux-Limited X-ray (REFLEX) catalog of galaxy clusters. The REFLEX survey covers 4.24 steradians (34% of th…

astro-ph2008★ 15 cited

The dynamical state of A548 from XMM-Newton data: X-ray and radio connection

L. Solovyeva, S. Anokhin, L. Feretti +5

We present a detailed study of the X-ray properties of the galaxy cluster Abell 548b (z=0.04), using XMM-Newton data, and discuss the connection between the thermal properties and…

astro-ph2007★ 11 cited

The distant galaxy cluster CL0016+16: X-ray analysis up to

L. Solovyeva, S. Anokhin, J. L. Sauvageot +2

To study the mass distribution of galaxy clusters up to their Virial radius, CL0016+16 seems to be a good candidate,since it is a bright massive cluster, previously considered as b…

astro-ph2006★ 2 cited

Tracing Ghost Cavities with Low Frequency Radio Observations

Tracy Clarke, Elizabeth Blanton, Craig Sarazin +5

We present X-ray and multi-frequency radio observations of the central radio sources in several X-ray cavity systems. We show that targeted radio observations are key to determinin…

astro-ph2006★ 24 cited

XMM-Newton observations of the Coma cluster relic 1253+275

Luigina Feretti, Doris M. Neumann

Using XMM Newton data, we investigate the nature of the X-ray emission in the radio relic 1253+275 in the Coma cluster. We determine the conditions of the cluster gas to check curr…

astro-ph2005★ 49 cited

Tracing the X-ray emitting intra-cluster medium of clusters of galaxies beyond r_200

D. M. Neumann

(Abridged) We present in this paper a sample of 14 nearby clusters of galaxies observed with the ROSAT/PSPC. We only select clusters with low galactic nH in order to trace the X-ra…