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19952021
most citedThe 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications

2.1k citations · 10.3k across the 81 of their papers we have counts for

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50 papers · 1 filter

astro-ph2008★ 55 cited

The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraints

Martin Sahlén, Pedro T. P. Viana, Andrew R. Liddle +16

We forecast the constraints on the values of sigma_8, Omega_m, and cluster scaling relation parameters which we expect to obtain from the XMM Cluster Survey (XCS). We assume a flat…

astro-ph2008★ 68 cited

The luminosity -- halo-mass relation for brightest cluster galaxies

Sarah Brough, Warrick Couch, Chris Collins +2

We examine the central-galaxy luminosity -- host-halo mass relation for 54 Brightest Group Galaxies (BGGs) and 92 Brightest Cluster Galaxies (BCGs) at z<0.1 and present the first m…

astro-ph2007★ 260 cited

The Representative XMM-Newton Cluster Structure Survey (REXCESS) of an X-ray Luminosity Selected Galaxy Cluster Sample

H. Boehringer, P. Schuecker, G. W. Pratt +31

The largest uncertainty for cosmological studies using clusters of galaxies is introduced by our limited knowledge of the statistics of galaxy cluster structure, and of the scaling…

astro-ph2005★ 22 cited

The 2dF Galaxy Redshift Survey: correlation with the ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey

Matt Hilton, Chris Collins, Roberto De Propris +25

The ROSAT-ESO Flux Limited X-ray (REFLEX) galaxy cluster survey and the 2dF Galaxy Redshift Survey (2dFGRS) respectively comprise the largest, homogeneous X-ray selected cluster ca…

astro-ph2005★ 54 cited

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

project: III. Gas mass fraction shape in high redshift clusters

Rachida Sadat, Alain Blanchard, Sebastien C. Vauclair +10

We study the gas mass fraction, behavior in project. The typical shape of high redshift galaxy clusters follows the global shape inf…