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Galaxy Clustering in the Completed SDSS Redshift Survey: The Dependence on Color and Luminosity

Journal Article · · Astrophys.J.
 [1];  [2];  [3];  [4];  [5];  [6];  [7];  [8];  [5];  [5];  [9];  [9];  [10];  [11];  [5];  [12];  [13]
  1. Case Western Reserve U.
  2. Yale U.
  3. Ohio State U.
  4. New York U.
  5. Princeton U.
  6. Vanderbilt U.
  7. Apache Point Observ.
  8. Chicago U.; Fermilab
  9. Portsmouth U.
  10. Penn State U.
  11. Arizona U.
  12. MIT
  13. Chicago U., EFI; Chicago U.
+ Show Author Affiliations
We measure the luminosity and color dependence of galaxy clustering in the SDSS DR7 main galaxy sample, focusing on the projected correlation function w_p(r_p) of volume-limited samples. We interpret our measurements using halo occupation distribution (HOD) modeling assuming a Lambda-CDM cosmology. The amplitude of w_p(r_p) grows slowly with luminosity for L < L_* and increases sharply at higher luminosities, with bias factor b(>L)=1.06+0.23(L/L_*)^{1.12}. At fixed luminosity, redder galaxies have a stronger and steeper w_p(r_p), a trend that runs steadily from the bluest galaxies to the reddest galaxies. The individual luminosity trends for the red and blue galaxy populations are strikingly different. Blue galaxies show a slow but steady increase of w_p(r_p) with luminosity, at all scales. The large-scale clustering of red galaxies shows little luminosity dependence until a sharp increase at L > 4L_*, but the lowest luminosity red galaxies (0.04-0.25 L_*) show very strong clustering on scales r_p < 2 Mpc/h. Most of the observed trends can be naturally understood within the LCDM+HOD framework. The growth of w_p(r_p) with luminosity reflects an overall shift in the halo mass scale, in particular an increase in the minimum host halo mass Mmin. The mass at which a halo has, on average, one satellite galaxy brighter than L is M_1 ~ 17 Mmin(L) over most of the luminosity range. The growth and steepening of w_p(r_p) for redder galaxies reflects the increasing fraction of galaxies that are satellite systems in high mass halos instead of central systems in low mass halos, a trend that is especially marked at low luminosities. Our extensive measurements, provided in tabular form, will allow detailed tests of theoretical models of galaxy formation, a firm grounding of semi-empirical models of the galaxy population, and new cosmological tests.
Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Contributing Organization:
SDSS
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1974018
Report Number(s):
FERMILAB-PUB-10-535-A; arXiv:1005.2413; oai:inspirehep.net:855689
Journal Information:
Astrophys.J., Journal Name: Astrophys.J. Vol. 736
Country of Publication:
United States
Language:
English

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