2XMM J083026+524133: the most X-ray luminous cluster at redshift 1

2008/07/01 by G. Lamer, M. Hoeft, J. Kohnert +2 · 4 citations
Physics and Astronomy · #Galaxies: Formation, Evolution, Phenomena #Astrophysical Phenomena and Observations #Astronomy and Astrophysical Research #Physics #Astrophysics #Redshift #Luminosity #Astronomy #Cluster (spacecraft) #Galaxy groups and clusters #Galaxy cluster #Galaxy #Population #Universe #Luminosity function

paper · pdf · doi:10.1051/0004-6361:200810255

openalex publication_date 2008/07/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

Aims. In the distant universe X-ray luminous clusters of galaxies are rare objects. Large area surveys are therefore needed to probe the high luminosity end of the cluster population at redshifts .

Citations

• Images, Structural Properties, and Metal Abundances of Galaxy Clusters Observed withChandraACIS‐I at 0.1 <z< 1.3
• H I in the Galaxy

Cited by

• The 3XMM/SDSS Stripe 82 Galaxy Cluster Survey
• AMI SZ observations and Bayesian analysis of a sample of six redshift-one clusters of galaxies
• XMMU J100750.5+125818: a strong lensing cluster atz= 1.082
• Lynx (constellation) [wikipedia]

Related

• The XXL Survey
• Galaxy population properties of the massive X-ray luminous galaxy cluster XDCP J0044.0-2033 atz= 1.58
• Studying Cosmic Evolution with the XMM-Newton Distant Cluster Project: X-ray Luminous Galaxy Clusters at z>~1 and their Galaxy Populations
• X-ray Surveys of Distant Galaxy Clusters
• 2XMM J100451.6+411627: A cool core cluster at z=0.82