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Discovery of a massive X-ray luminous galaxy cluster at z=1.579

  • Santos, Joana S.
  • Fassbender, Rene
  • Nastasi, Alessandro
  • Böhringer, Hans
  • Rosati, Piero
  • Suhada, Robert
  • Pierini, Daniele
  • Nonino, Mario
  • Muehlegger, Martin
  • Quintana, Hernan
  • Schwope, Axel D.
  • Lamer, Georg
  • de Hoon, Arjen
  • Strazzullo, Veronica
Publication Date
May 30, 2011
Submission Date
May 30, 2011
DOI: 10.1051/0004-6361/201117190
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We report on the discovery of a very distant galaxy cluster serendipitously detected in the archive of the XMM-Newton mission, within the scope of the XMM-Newton Distant Cluster Project (XDCP). XMMUJ0044.0-2033 was detected at a high significance level (5sigma) as a compact, but significantly extended source in the X-ray data, with a soft-band flux f(r<40")=(1.5+-0.3)x10^(-14) erg/s/cm2. Optical/NIR follow-up observations confirmed the presence of an overdensity of red galaxies matching the X-ray emission. The cluster was spectroscopically confirmed to be at z=1.579 using ground-based VLT/FORS2 spectroscopy. The analysis of the I-H colour-magnitude diagram shows a sequence of red galaxies with a colour range [3.7 < I-H < 4.6] within 1' from the cluster X-ray emission peak. However, the three spectroscopic members (all with complex morphology) have significantly bluer colours relative to the observed red-sequence. In addition, two of the three cluster members have [OII] emission, indicative of on-going star formation. Using the spectroscopic redshift we estimated the X-ray bolometric luminosity, Lbol = 5.8x10^44 erg/s, implying a massive galaxy cluster. This places XMMU J0044.0-2033 at the forefront of massive distant clusters, closing the gap between lower redshift systems and recently discovered proto- and low-mass clusters at z >1.6.

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