THE CLUSTERING OF GALAXIES IN THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY: LUMINOSITY AND COLOR DEPENDENCE AND REDSHIFT EVOLUTION

被引:79
作者
Guo, Hong [1 ,2 ]
Zehavi, Idit [1 ]
Zheng, Zheng [2 ]
Weinberg, David H. [3 ,4 ]
Berlind, Andreas A. [5 ]
Blanton, Michael [6 ]
Chen, Yanmei [7 ]
Eisenstein, Daniel J. [8 ]
Ho, Shirley [9 ,10 ]
Kazin, Eyal [11 ]
Manera, Marc [12 ]
Maraston, Claudia [12 ,13 ]
McBride, Cameron K. [8 ]
Nuza, Sebastian E. [14 ]
Padmanabhan, Nikhil [15 ]
Parejko, John K. [15 ]
Percival, Will J. [12 ]
Ross, Ashley J. [12 ]
Ross, Nicholas P. [9 ]
Samushia, Lado [12 ,16 ]
Sanchez, Ariel G. [17 ]
Schlegel, David J. [9 ]
Schneider, Donald P. [18 ,19 ]
Skibba, Ramin A. [20 ]
Swanson, Molly E. C. [8 ]
Tinker, Jeremy L. [6 ]
Tojeiro, Rita [12 ]
Wake, David A. [21 ,22 ]
White, Martin [9 ,23 ,24 ]
Bahcall, Neta A. [25 ]
Bizyaev, Dmitry [26 ]
Brewington, Howard [26 ]
Bundy, Kevin [27 ]
da Costa, Luiz N. A. [28 ,29 ]
Ebelke, Garrett [26 ]
Malanushenko, Elena [26 ]
Malanushenko, Viktor [26 ]
Oravetz, Daniel [26 ]
Rossi, Graziano [30 ,31 ,32 ]
Simmons, Audrey [26 ]
Snedden, Stephanie [26 ]
Streblyanska, Alina [33 ,34 ]
Thomas, Daniel [12 ,13 ]
机构
[1] Case Western Reserve Univ, Dept Astron, Cleveland, OH 44106 USA
[2] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA
[3] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
[4] Ohio State Univ, CCAPP, Columbus, OH 43210 USA
[5] Vanderbilt Univ, Dept Phys & Astron, Nashville, TN 37235 USA
[6] NYU, Ctr Cosmol & Particle Phys, New York, NY 10003 USA
[7] Nanjing Univ, Dept Astron, Nanjing 210093, Jiangsu, Peoples R China
[8] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
[9] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
[10] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA
[11] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[12] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
[13] SEPnet, South East Phys Network, Highfield, England
[14] Leibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, Germany
[15] Yale Univ, Dept Phys, New Haven, CT 06520 USA
[16] Ilia State Univ, Natl Abastumani Astrophys Observ, GE-1060 Tbilisi, Georgia
[17] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[18] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[19] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
[20] Univ Calif San Diego, Ctr Astrophys & Space Sci, San Diego, CA 92093 USA
[21] Yale Univ, Dept Astron, New Haven, CT 06520 USA
[22] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA
[23] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[24] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[25] Princeton Univ Observ, Princeton, NJ 08544 USA
[26] Apache Point Observ, Sunspot, NM 88349 USA
[27] Univ Tokyo, Kavli Inst Phys & Math Universe, Kashiwa, Chiba 2778582, Japan
[28] Observ Nacl, BR-20921400 Rio De Janeiro, RJ, Brazil
[29] Lab Interinst E Astron LineA, BR-20921400 Rio De Janeiro, RJ, Brazil
[30] CEA, Ctr Saclay, Irfu SPP, F-91191 Gif Sur Yvette, France
[31] Univ Paris 07, Paris Ctr Cosmol Phys PCCP, F-75205 Paris, France
[32] Univ Paris 07, Lab APC, F-75205 Paris, France
[33] Inst Astrofis Canarias, E-38200 Tenerife, Spain
[34] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
基金
美国国家科学基金会;
关键词
cosmology: observations; cosmology: theory; galaxies: distances and redshifts; galaxies: halos galaxies: statistics; large-scale structure of universe; DIGITAL SKY SURVEY; HALO OCCUPATION DISTRIBUTION; MEDIUM-BAND SURVEY; VLT DEEP SURVEY; RED GALAXIES; 2DF-SDSS LRG; MAGNITUDE RELATION; STELLAR EVOLUTION; ANALYTIC MODEL; REAL-SPACE;
D O I
10.1088/0004-637X/767/2/122
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We measure the luminosity and color dependence and the redshift evolution of galaxy clustering in the Sloan Digital Sky Survey-III Baryon Oscillation Spectroscopic Survey Ninth Data Release. We focus on the projected two-point correlation function (2PCF) of subsets of its CMASS sample, which includes about 260,000 galaxies over similar to 3300 deg(2) in the redshift range 0.43 < z < 0.7. To minimize the selection effect on galaxy clustering, we construct well-defined luminosity and color subsamples by carefully accounting for the CMASS galaxy selection cuts. The 2PCF of the whole CMASS sample, if approximated by a power-law, has a correlation length of r(0) = 7.93 +/- 0.06 h(-1) Mpc and an index of gamma = 1.85 +/- 0.01. Clear dependences on galaxy luminosity and color are found for the projected 2PCF in all redshift bins, with more luminous and redder galaxies generally exhibiting stronger clustering and steeper 2PCF. The color dependence is also clearly seen for galaxies within the red sequence, consistent with the behavior of SDSS-II main sample galaxies at lower redshifts. At a given luminosity (k + e corrected), no significant evolution of the projected 2PCFs with redshift is detected for red sequence galaxies. We also construct galaxy samples of fixed number density at different redshifts, using redshiftdependent magnitude thresholds. The clustering of these galaxies in the CMASS redshift range is found to be consistent with that predicted by passive evolution. Our measurements of the luminosity and color dependence and redshift evolution of galaxy clustering will allow for detailed modeling of the relation between galaxies and dark matter halos and new constraints on galaxy formation and evolution.
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页数:19
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