4.6 Article

Groups and clusters of galaxies in the SDSS DR8 Value-added catalogues

Journal

ASTRONOMY & ASTROPHYSICS
Volume 540, Issue -, Pages -

Publisher

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201118687

Keywords

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

Funding

  1. Estonian Science Foundation [7765, 8005, 9428, MJD272]
  2. Estonian Ministry for Education and Science [SF0060067s08]
  3. Centre of Excellence of Dark Matter in (Astro) particle Physics and Cosmology [TK120]
  4. University of Valencia
  5. Generalitat Valenciana [PROMETEO/2009/064]
  6. Alfred P. Sloan Foundation
  7. National Science Foundation
  8. US Department of Energy Office of Science
  9. University of Arizona
  10. Brazilian Participation Group
  11. Brookhaven National Laboratory
  12. University of Cambridge
  13. University of Florida
  14. French Participation Group
  15. German Participation Group
  16. Instituto de Astrofisica de Canarias
  17. Michigan State/Notre Dame/JINA Participation Group
  18. Johns Hopkins University
  19. Lawrence Berkeley National Laboratory
  20. Max Planck Institute for Astrophysics
  21. New Mexico State University
  22. New York University
  23. Ohio State University
  24. Pennsylvania State University
  25. University of Portsmouth
  26. Princeton University
  27. Spanish Participation Group
  28. University of Tokyo
  29. University of Utah
  30. Vanderbilt University
  31. University of Virginia
  32. University of Washington
  33. Yale University

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Aims. We intend to compile a new galaxy group and cluster sample of the latest available SDSS data, adding several parameter for the purpose of studying the supercluster network, galaxy and group evolution, and their connection to the surrounding environment. Methods. We used a modified friends-of-friends (FoF) method with a variable linking length in the transverse and radial directions to eliminate selection effects and to find reliably as many groups as possible. Using the galaxies as a basis, we calculated the luminosity density field. Results. We create a new catalogue of groups and clusters for the SDSS data release 8 sample. We find and add environmental parameters to our catalogue, together with other galaxy parameters (e.g., morphology), missing from our previous catalogues. We take into account various selection effects caused by a magnitude limited galaxy sample. Our final sample contains 576 493 galaxies and 77 858 groups.

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