SXDF X-ray groups and galaxy clusters (Finoguenov+, 2010)

A. Finoguenov, M. G. Watson, M. Tanaka, C. Simpson, M. Cirasuolo, J. S. Dunlop, J. A. Peacock, D. Farrah, M. Akiyama, Y. Ueda, V. Smolcic, G. Stewart, S. Rawlings, C. van Breukelen, O. Almaini, L. Clewley, D. G. Bonfield, M. J. Jarvis, J. M. Barr, S. FoucaudR. J. McLure, K. Sekiguchi, E. Egami

Research output: Contribution to journalArticlepeer-review


We present the results of a search for galaxy clusters in the Subaru-XMM Deep Field (SXDF). We reach a depth for a total cluster flux in the 0.5-2keV band of 2x10-15erg/cm2/s over one of the widest XMM-Newton contiguous raster surveys, covering an area of 1.3deg2. Cluster candidates are identified through a wavelet detection of extended X-ray emission. The red-sequence technique allows us to identify 57 cluster candidates. We report on the progress with the cluster spectroscopic follow-up and derive their properties based on the X-ray luminosity and cluster scaling relations. (3 data files).
Original languageEnglish
Pages (from-to)32063
JournalVizieR On-line Data Catalog
Publication statusPublished - 1 Feb 2012


  • Surveys
  • X-ray sources
  • Clusters: galaxy


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