First simultaneous optical/near-infrared imaging of an X-ray selected, high-redshift cluster of galaxies with GROND

The galaxy population of XMMU J0338.7 + 0030 at z = 1.1^⋆

¹ Max-Planck-Institut für extraterrestrische Physik (MPE), Giessenbachstrasse, 85748 Garching, Germany
e-mail: dpierini@mpe.mpg.de
² University Observatory Munich, Scheinerstrasse 1, 81679 Munich, Germany
³ Max-Planck-Institut für Plasmaphysik, Boltzmannstrasse 2, 85748 Garching, Germany
⁴ Caltech, 1200 East California Blvd, PMA 249-17, Pasadena, CA 91125, USA
⁵ Laboratoire AIM, IRFU/Service d’Astrophysique – CEA/DSM – CNRS – Université Paris Diderot, Bât. 709, CEA-Saclay, 91191 Gif-sur-Yvette Cedex, France
⁶ European Southern Observatory (ESO), Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany
⁷ European Space Astronomy Centre (ESAC), PO Box 78, 28691 Villanueva de la Cañada, Madrid, Spain
⁸ Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany
⁹ Department of Physics, Ludwig-Maximilians-Universität, Scheinerstrasse 1, 81679 Munich, Germany
¹⁰ Excellence Cluster Universe, Boltzmannstrasse 2, 85748 Garching, Germany
¹¹ Departamento de Astronomía y Astrofísica, Pontificia Universidad Católica de Chile, Casilla 306, Santiago 22, Chile
¹² Leiden Observatory, PO Box 9513, 2300 RA Leiden, The Netherlands
¹³ American River College, Physics and Astronomy Dept., 4700 College Oak Drive, Sacramento, CA 95841, USA
¹⁴ Dark Cosmology Centre, Niels Bohr Institute, University of Copenhagen, Juliane Maries Vej 30, 2100 Cøbenhavn Ø, Denmark
¹⁵ Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 0HA, UK
¹⁶ Thüringer Landessternwarte Tautenburg, Sternwarte 5, 07778 Tautenburg, Germany

Received: 8 February 2011
Accepted: 13 December 2011

Abstract

Context. The XMM-Newton Distant Cluster Project is a serendipitous survey for clusters of galaxies at redshifts z ≥ 0.8 based on deep archival XMM-Newton observations. X-ray sources identified as extended are screened against existing optical all-sky surveys for galaxies, in case of candidate high-z clusters followed up with imaging at 4 m-class telescopes and, ultimately, multi-object spectroscopy at 8 m-class telescopes. Low-significance candidate high-z clusters are followed up with the seven-channel imager GROND (Gamma-Ray Burst Optical and Near-Infrared Detector) that is mounted at a 2 m-class telescope. Its unique capability of simultaneous imaging in the g′,r′,i′,z′,J,H,Ks bands enables the use of the photometric redshift technique.

Aims. Observing strategy, data reduction and analysis, depth and accuracy of the simultaneous multi-wavelength photometry are discussed with the goal of establishing GROND as a useful instrument to confirm X-ray selected (high-z) clusters.

Methods. The test case is XMMU J0338.7 + 0030, suggested to be at z ~ 1.45 ± 0.15 (1σ) from the analysis of the z − H vs. H colour − magnitude diagram obtained from the follow-up imaging. Later VLT-FORS2 spectroscopy enabled us to identify four members, which set this cluster at z = 1.097 ± 0.002 (1σ). To reach a better knowledge of its galaxy population, we observed XMMU J0338.7 + 0030 with GROND for about 6   h. The publicly available photo-z code le Phare was used.

Results. The Ks-band number counts of the non-stellar sources out of the 832 detected down to z′ ~ 26   AB   mag (1σ) in the 3.9 × 4.3   arcmin² region of XMMU J0338.7 + 0030 imaged at all GROND bands clearly exceed those computed in deep fields/survey areas at  ~20.5–22.5 AB mag. The photo-z’s of the three imaged spectroscopic members yield z = 1.12 ± 0.09 (1σ). The spatial distribution and the properties of the GROND sources with a photo-z in the range 1.01–1.23 confirm the correspondence of the X-ray source with a galaxy over-density at a significance of at least 4.3σ. Candidate members that are spectro-photometrically classified as elliptical galaxies define a red locus in the i′ − z′ vs. z′ colour − magnitude diagram that is consistent with the red sequence of the cluster RDCS J0910 + 5422 at z = 1.106. XMMU J0338.7 + 0030 hosts also a population of bluer late-type spirals and irregulars. The starbursts among the photometric members populate both loci, consistently with previous results.

Conclusions. The analysis of the available data set indicates that XMMU J0338.7 + 0030 is a low-mass cluster (M₂₀₀ ~ 10¹⁴   M_⊙) at z = 1.1. With the photometric accuracy yielded by the present unoptimized multi-band observations with GROND, we not only confirm the spectroscopic redshift of this cluster but also show that it hosts a galaxy population that can still undergo significant bursts of star-formation activity.