Indications for 3 Mpc-scale large-scale structure associated with an X-ray luminous cluster of galaxies at z = 0.95

2008/02/19 by R. Fassbender, H. Boehringer, H. Böhringer +7 · 1 citation
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysical Phenomena and Observations #Astrophysics #COSMIC cancer database #Cluster (spacecraft) #Computer science #Context (archaeology) #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Galaxy formation and evolution #Geography #Physics #Scale (ratio) #astro-ph

paper · pdf · doi:10.1051/0004-6361:20079001

5 pages, 4 figures, accepted for publication in A&A

arxiv created 2008/02/19 · openalex publication_date 2008/02/20 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Context. X-ray luminous clusters of galaxies at z ~ 1 are emerging as major cosmological probes and are fundamental tools to study the cosmic large-scale structure and environmental effects of galaxy evolution at large look-back times.

Citations

• The NRAO VLA Sky Survey
• Radio Sources in Galaxy Clusters: Radial Distribution, and 1.4 GHz andK‐band Bivariate Luminosity Function
• H I in the Galaxy
• Galaxy populations of double cluster RX J1053.7+5735 at z = 1.13
• Entropy scaling in galaxy clusters: Insights from anXMM-Newtonobservation of the poor cluster A1983
• The Color‐Magnitude Relation in CL 1358+62 atz= 0.33: Evidence for Significant Evolution in the S0 Population

Cited by

• XMMU J100750.5+125818: a strong lensing cluster atz= 1.082