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The XMM Cluster Survey: Present status and latest results

Research output: Contribution to journalJournal articlepeer-review

Published
  • P. T P Viana
  • N. Mehrtens
  • C. D. Harrison
  • A. K. Romer
  • C. A. Collins
  • M. Hilton
  • B. Hoyle
  • S. T. Kay
  • A. R. Liddle
  • J. A. Mayers
  • C. J. Miller
  • P. J. Rooney
  • M. Sahlén
  • J. P. Stott
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<mark>Journal publication date</mark>05/2013
<mark>Journal</mark>Astronomical Notes / Astronomische Nachrichten
Issue number4-5
Volume334
Number of pages4
Pages (from-to)462-465
Publication StatusPublished
Early online date2/05/13
<mark>Original language</mark>English

Abstract

The XMM Cluster Survey (XCS) is a serendipitous search for galaxy clusters using all publicly available data in the XMM-Newton Science Archive. Our recent first data release (XCS-DR1) contains 503 optically confirmed groups and clusters, among which 256 new to the literature and 357 whose X-ray emission was detected for the first time. We discuss their properties and provide an update on the work being done. As examples of the applications of XCS-DR1, we mention the 17 fossil groups/clusters identified with the help of the Sloan Digital Sky Survey. Their brightest galaxies have stellar populations and star-formation histories which are similar to normal brightest cluster galaxies, but their stellar masses are significantly larger and correspond to a much bigger fraction of the total group/cluster optical luminosity. We also highlight the 15 clusters expected tobe also detected by the Planck satellite, and characterize the expected overlap between the final XCS and Planck cluster catalogues.