94 citations · 500 across the 22 of their papers we have counts for
8 papers · 1 filter
Probing the dynamical and X-ray mass proxies of the cluster of galaxies Abell S1101
Andreas Rabitz, Yu-Ying Zhang, Axel Schwope +3
Context: The galaxy cluster Abell S1101 (S1101 hereafter) deviates significantly from the X-ray luminosity versus velocity dispersion relation (L-sigma) of galaxy clusters in our p…
Kinematic analysis of a sample of X-ray luminous distant galaxy clusters. The - relation in the universe
Alessandro Nastasi, Hans Böhringer, Rene Fassbender +11
Observations and cosmological simulations show galaxy clusters as a family of nearly self-similar objects with properties that can be described by scaling relations as a function o…
Distant galaxy clusters in a deep XMM-Newton field within the CFTHLS D4
Arjen de Hoon, Georg Lamer, Axel Schwope +15
The XMM-Newton Distant Cluster Project (XDCP) aims at the identification of a well defined sample of X-ray selected clusters of galaxies at redshifts z>0.8. We present a catalogue…
Probing cluster dynamics in RXCJ1504.1-0248 via radial and two-dimensional gas and galaxy properties
Yu-Ying Zhang, Miguel Verdugo, Matthias Klein +1
We studied one of the most X-ray luminous cluster of galaxies in the REFLEX survey, RXC J1504.1-0248 (hereafter R1504; z=0.2153), using XMM-Newton X-ray imaging spectroscopy, VLT/V…
First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND: the galaxy population of XMMU J0338.7+0030 at z=1.1
D. Pierini, R. Suhada, R. Fassbender +28
The XMM-Newton Distant Cluster Project is a serendipitous survey for clusters of galaxies at redshifts z>=0.8 based on deep archival XMM-Newton observations. ... Low-significance c…
The Cosmic Web and galaxy evolution around the most luminous X-ray cluster: RXJ1347.5-1145
M. Verdugo, M. Lerchster, H. Boehringer +5
In this paper we study the large scale structures and their galaxy content around the most X-ray luminous cluster known, RX J1347.5-1145 at z=0.45. We make use of ugriz CFHT MEGACA…