The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples

被引：1253

作者：

Anderson, Lauren ^{[1
]}

Aubourg, Eric ^{[2
]}

Bailey, Stephen ^{[3
]}

Beutler, Florian ^{[3
]}

Bhardwaj, Vaishali ^{[1
,3
]}

Blanton, Michael ^{[4
]}

Bolton, Adam S. ^{[5
]}

Brinkmann, J. ^{[6
]}

Brownstein, Joel R. ^{[5
]}

Burden, Angela ^{[7
]}

Chuang, Chia-Hsun ^{[8
]}

Cuesta, Antonio J. ^{[9
,10
]}

Dawson, Kyle S. ^{[5
]}

Eisenstein, Daniel J. ^{[11
]}

Escoffier, Stephanie ^{[12
]}

Gunn, James E. ^{[13
]}

Guo, Hong ^{[5
]}

Ho, Shirley ^{[14
]}

Honscheid, Klaus ^{[15
,16
]}

Howlett, Cullan ^{[7
]}

Kirkby, David ^{[17
]}

Lupton, Robert H. ^{[14
]}

Manera, Marc ^{[7
,18
]}

Maraston, Claudia ^{[7
]}

McBride, Cameron K. ^{[11
]}

Mena, Olga ^{[19
]}

Montesano, Francesco ^{[20
]}

Nichol, Robert C. ^{[7
]}

Nuza, Sebastian E. ^{[21
]}

Olmstead, Matthew D. ^{[5
]}

Padmanabhan, Nikhil ^{[9
]}

Palanque-Delabrouille, Nathalie ^{[3
,22
]}

Parejko, John ^{[9
]}

Percival, Will J. ^{[7
]}

Petitjean, Patrick ^{[23
]}

Prada, Francisco ^{[8
,24
,25
]}

Price-Whelan, Adrian M. ^{[26
]}

Reid, Beth ^{[3
,27
]}

Roe, Natalie A. ^{[3
]}

Ross, Ashley J. ^{[7
]}

Ross, Nicholas P. ^{[3
,28
]}

Sabiu, Cristiano G. ^{[29
]}

Saito, Shun ^{[30
]}

Samushia, Lado ^{[7
,31
]}

Sanchez, Ariel G. ^{[20
]}

Schlegel, David J. ^{[3
]}

Schneider, Donald P. ^{[32
,33
]}

Scoccola, Claudia G. ^{[8
,34
,35
]}

Seo, Hee-Jong ^{[16
,36
,37
]}

Skibba, Ramin A. ^{[38
]}

机构：

[1] Univ Washington, Dept Astron, Seattle, WA 98195 USA

[2] Univ Paris Diderot, CNRS IN2P3, CEA Irfu, APC,Observ Paris,Sorbonne Paris Cite, F-75205 Paris 13, France

[3] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA

[4] NYU, Ctr Cosmol & Particle Phys, New York, NY 10003 USA

[5] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA

[6] Apache Point Observ, Sunspot, NM 88349 USA

[7] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England

[8] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain

[9] Yale Univ, Dept Phys, New Haven, CT 06520 USA

[10] Univ Barcelona, IEEC UB, Inst Ciencies Cosmos, E-08028 Barcelona, Spain

[11] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA

[12] Aix Marseille Univ, CPPM, CNRS IN2P3, Marseille 07, France

[13] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[14] Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA

[15] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA

[16] Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA

[17] UC Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

[18] UCL, London WC1E 6BT, England

[19] Univ Valencia, IFIC, CSIC, E-46071 Valencia, Spain

[20] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany

[21] Leibniz Inst Astrophys Potsdam AIP, D-14482 Potsdam, Germany

[22] CEA, Ctr Saclay, IRFU, F-91191 Gif Sur Yvette, France

[23] Univ Paris 06, Inst Astrophys Paris, CNRS UMR7095, F-75014 Paris, France

[24] Campus Int Excellence UAM CSIC, E-28049 Madrid, Spain

[25] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain

[26] Columbia Univ, Dept Astron, New York, NY 10027 USA

[27] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[28] Drexel Univ, Dept Phys, Philadelphia, PA 19104 USA

[29] Korea Inst Adv Study, Seoul 130722, South Korea

[30] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, Todai Inst Adv Study, Chiba 2778582, Japan

[31] Ilia State Univ, Natl Abastumani Astrophys Observ, GE-1060 Tbilisi, Georgia

[32] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA

[33] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA

[34] IAC, E-38200 Tenerife, Spain

[35] Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain

[36] Univ Calif Berkeley, Berkeley Ctr Cosmol Phys, LBL, Berkeley, CA 94720 USA

[37] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA

[38] Univ Calif San Diego, Dept Phys, Ctr Astrophys & Space Sci, San Diego, CA 92093 USA

[39] ICREA, E-08028 Barcelona, Spain

[40] ICC UB Univ Barcelona, E-08028 Barcelona, Spain

[41] Univ Wisconsin, Dept Astron, Madison, WI 53706 USA

[42] Open Univ, Dept Phys Sci, Milton Keynes MK7 6AA, Bucks, England

[43] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA

[44] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA

[45] Case Western Reserve Univ, Dept Astron, Cleveland, OH 44106 USA

[46] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2014年 / 441卷 / 01期

基金：

美国安德鲁·梅隆基金会; 美国国家科学基金会;

关键词：

cosmological parameters; cosmology: observations; dark energy; distance scale; large-scale structure of Universe; DIGITAL SKY SURVEY; POWER-SPECTRUM ANALYSIS; HUBBLE-SPACE-TELESCOPE; LUMINOUS RED GALAXIES; CENT DISTANCE; TO; 0.5; SCALE; CALIBRATION; EVOLUTION; UNIVERSE;

D O I：

10.1093/mnras/stu523

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a one per cent measurement of the cosmic distance scale from the detections of the baryon acoustic oscillations (BAO) in the clustering of galaxies from the Baryon Oscillation Spectroscopic Survey, which is part of the Sloan Digital Sky Survey III. Our results come from the Data Release 11 (DR11) sample, containing nearly one million galaxies and covering approximately 8500 square degrees and the redshift range 0.2 < z < 0.7. We also compare these results with those from the publicly released DR9 and DR10 samples. Assuming a concordance A cold dark matter (ACDM) cosmological model, the DR11 sample covers a volume of 13 Gpc(3) and is the largest region of the Universe ever surveyed at this density. We measure the correlation function and power spectrum, including density- field reconstruction of the BAO feature. The acoustic features are detected at a significance of over 7s in both the correlation function and power spectrum. Fitting for the position of the acoustic features measures the distance relative to the sound horizon at the drag epoch, r(d), which has a value of r(d,fid) = 149.28 Mpc in our fiducial cosmology. We find D-V = (1264 +/- 25 Mpc)(r(d)/r(d,fid)) at z = 0.32 and D-V = (2056 +/- 20 Mpc)(r(d)/r(d,fid)) at z = 0.57. At 1.0 per cent, this latter measure is the most precise distance constraint ever obtained from a galaxy survey. Separating the clustering along and transverse to the line of sight yields measurements at z = 0.57 of D-A = (1421 +/- 20 Mpc)(r(d)/r(d,fid)) and H = (96.8 +/- 3.4 kms(-1) Mpc(-1))(r(d),(fid)/r(d)). Our measurements of the distance scale are in good agreement with previous BAO measurements and with the predictions from cosmic microwave background data for a spatially flat CDM model with a cosmological constant.

引用

页码：24 / 62

页数：39

共 131 条

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← 1 2 3 4 5 6 7 8 9 10 →

共 131 条

[1] The second data release of the Sloan Digital Sky Survey [J].

Abazajian, K ;

Adelman-McCarthy, JK ;

Agüeros, MA ;

Allam, SS ;

Kurt ;

Anderson, SJ ;

Anderson, SF ;

Annis, J ;

Bahcall, NA ;

Baldry, IK ;

Bastian, S ;

Berlind, A ;

Bernardi, M ;

Blanton, MR ;

Bochanski, JJ ;

Boroski, WN ;

Briggs, JW ;

Brinkmann, J ;

Brunner, RJ ;

Budavári, T ;

Carey, LN ;

Carliles, S ;

Castander, FJ ;

Connolly, AJ ;

Csabai, I ;

Doi, M ;

Dong, F ;

Eisenstein, DJ ;

Evans, ML ;

Fan, XH ;

Finkbeiner, DP ;

Friedman, SD ;

Frieman, JA ;

Fukugita, M ;

Gal, RR ;

Gillespie, B ;

Glazebrook, K ;

Gray, J ;

Grebel, EK ;

Gunn, JE ;

Gurbani, VK ;

Hall, PB ;

Hamabe, M ;

Harris, FH ;

Harris, HC ;

Harvanek, M ;

Heckman, TM ;

Hendry, JS ;

Hennessy, GS ;

Hindsley, RB .

ASTRONOMICAL JOURNAL, 2004, 128 (01) :502-512

[2] THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY [J].

Abazajian, Kevork N. ;

Adelman-McCarthy, Jennifer K. ;

Agueros, Marcel A. ;

Allam, Sahar S. ;

Prieto, Carlos Allende ;

An, Deokkeun ;

Anderson, Kurt S. J. ;

Anderson, Scott F. ;

Annis, James ;

Bahcall, Neta A. ;

Bailer-Jones, C. A. L. ;

Barentine, J. C. ;

Bassett, Bruce A. ;

Becker, Andrew C. ;

Beers, Timothy C. ;

Bell, Eric F. ;

Belokurov, Vasily ;

Berlind, Andreas A. ;

Berman, Eileen F. ;

Bernardi, Mariangela ;

Bickerton, Steven J. ;

Bizyaev, Dmitry ;

Blakeslee, John P. ;

Blanton, Michael R. ;

Bochanski, John J. ;

Boroski, William N. ;

Brewington, Howard J. ;

Brinchmann, Jarle ;

Brinkmann, J. ;

Brunner, Robert J. ;

Budavari, Tamas ;

Carey, Larry N. ;

Carliles, Samuel ;

Carr, Michael A. ;

Castander, Francisco J. ;

Cinabro, David ;

Connolly, A. J. ;

Csabai, Istvan ;

Cunha, Carlos E. ;

Czarapata, Paul C. ;

Davenport, James R. A. ;

de Haas, Ernst ;

Dilday, Ben ;

Doi, Mamoru ;

Eisenstein, Daniel J. ;

Evans, Michael L. ;

Evans, N. W. ;

Fan, Xiaohui ;

Friedman, Scott D. ;

Frieman, Joshua A. .

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Ausse, H. ;

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Bartlett, J. G. ;

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Benoit, A. ;

Benoit-Levy, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bertincourt, B. ;

Bethermin, M. ;

Bielewicz, P. ;

Bikmaev, I. ;

Blanchard, A. ;

Bobin, J. ;

Bock, J. J. ;

Boehringer, H. ;

Bonaldi, A. ;

Bonavera, L. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Boulanger, F. ;

Bourdin, H. ;

Bowyer, J. W. ;

Bridges, M. ;

Brown, M. L. ;

Bucher, M. ;

Burenin, R. ;

Burigana, C. ;

Butler, R. C. ;

Calabrese, E. ;

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