Published June 1, 2009 | Version v1
Journal article

AN OPTICAL GROUP CATALOG TO z = 1 FROM THE zCOSMOS 10 k SAMPLE

  • 1. Institute of Astronomy, ETH Zurich (Switzerland)
  • 2. INAF Osservatorio Astronomico di Brera, Milan (Italy)
  • 3. INAF Osservatorio Astronomico di Bologna, via Ranzani 1, I-40127 Bologna (Italy)
  • 4. Max Planck Institute of Astrophysics, Karl-Schwarzschild Str. 1, P.O. Box 1317, D-85748 Garching (Germany)
  • 5. Laboratoire d'Astrophysique de Toulouse-Tarbes, Universite de Toulouse, CNRS, 14 avenue Edouard Belin, F-31400 Toulouse (France)
  • 6. Laboratoire d'Astrophysique de Marseille, Marseille (France)
  • 7. European Southern Observatory, Karl-Schwarzschild- Strasse 2, Garching, D-85748 (Germany)
  • 8. Dipartimento di Astronomia, Universita di Padova, Padova (Italy)
  • 9. INAF - IASF Milano, Milan (Italy)
  • 10. Max-Planck-Institut fuer extraterrestrische Physik, D-84571 Garching (Germany)

Description

We present a galaxy group catalog spanning the redshift range 0.1 ∼< z ∼< 1 in the ∼ 1.7 deg2 COSMOS field, based on the first ∼10,000 zCOSMOS spectra. The performance of both the Friends-of-Friends (FOF) and Voronoi-Delaunay method (VDM) approaches to group identification has been extensively explored and compared using realistic mock catalogs. We find that the performance improves substantially if groups are found by progressively optimizing the group-finding parameters for successively smaller groups, and that the highest fidelity catalog, in terms of completeness and purity, is obtained by combining the independently created FOF and VDM catalogs. The final completeness and purity of this catalog, both in terms of the groups and of individual members, compares favorably with recent results in the literature. The current group catalog contains 102 groups with N ≥ 5 spectroscopically confirmed members, with a further ∼700 groups with 2 ≤ N ≤ 4. Most of the groups can be assigned a velocity dispersion and a dark-matter mass derived from the mock catalogs, with quantifiable uncertainties. The fraction of zCOSMOS galaxies in groups is about 25% at low redshift and decreases toward ∼15% at z ∼ 0.8. The zCOSMOS group catalog is broadly consistent with that expected from the semianalytic evolution model underlying the mock catalogs. Not least, we show that the number density of groups with a given intrinsic richness increases from redshift z ∼ 0.8 to the present, consistent with the hierarchical growth of structure.

Availability note (English)

Available from http://dx.doi.org/10.1088/0004-637X/697/2/1842

Additional details

Identifiers

Publishing Information

Journal Title
Astrophysical Journal
Journal Volume
697
Journal Issue
2
Journal Page Range
p. 1842-1860
ISSN
0004-637X
CODEN
ASJOAB

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41051823
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
DATA ANALYSIS; GALAXIES; GALAXY CLUSTERS; MASS; MATHEMATICAL EVOLUTION; NONLUMINOUS MATTER; RED SHIFT; UNIVERSE
Descriptors DEC
EVOLUTION; MATTER