4.6 Article

Flux- and volume-limited groups/clusters for the SDSS galaxies: catalogues and mass estimation

Journal

ASTRONOMY & ASTROPHYSICS
Volume 566, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201423585

Keywords

galaxies: clusters: general; galaxies: groups: general; galaxies: statistics; large-scale structure of Universe; cosmology: observations; catalogs

Funding

  1. Estonian Research Council [9428, MJD272, PUT246, IUT26]
  2. Centre of Excellence of Dark Matter in (Astro)particle Physics and Cosmology
  3. Alfred P. Sloan Foundation
  4. National Science Foundation
  5. US Department of Energy Office of Science
  6. University of Arizona
  7. Brazilian Participation Group
  8. Brookhaven National Laboratory
  9. Carnegie Mellon University
  10. University of Florida
  11. French Participation Group
  12. German Participation Group
  13. Harvard University
  14. Instituto de Astrofisica de Canarias
  15. Michigan State/Notre Dame/JINA Participation Group
  16. Johns Hopkins University
  17. Lawrence Berkeley National Laboratory
  18. Max Planck Institute for Astrophysics
  19. Max Planck Institute for Extraterrestrial Physics
  20. New Mexico State University
  21. New York University
  22. Ohio State University
  23. Pennsylvania State University
  24. University of Portsmouth
  25. Princeton University
  26. Spanish Participation Group
  27. University of Tokyo
  28. University of Utah
  29. Vanderbilt University
  30. University of Virginia
  31. University of Washington
  32. Yale University

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We provide flux-and volume-limited galaxy group and cluster catalogues based on the spectroscopic sample of the galaxies of SDSS data release 10. We used a modified friends-of-friends method with a variable linking length in the transverse and radial directions to identify as many realistic groups as possible. The flux-limited catalogue incorporates galaxies down to m(r) = 17.77 mag. It includes 588 193 galaxies and 82 458 groups. The volume-limited catalogues are complete for absolute magnitudes down to M-r,M-lim = -18.0, -18.5, -19.0, -19.5, -20.0, -20.5, and -21.0; the completeness is achieved within different spatial volumes. Our analysis shows that flux-and volume-limited group samples are well compatible, especially for the larger groups/clusters. Dynamical mass estimates based on radial velocity dispersions and group extent in the sky were added to the extracted groups.

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