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The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples
文献类型：期刊论文
| 作者 | Anderson, Lauren1; Aubourg, Eric2; Bailey, Stephen3; Beutler, Florian3; Bhardwaj, Vaishali1,3; Blanton, Michael4; Bolton, Adam S.5; Brinkmann, J.6; Brownstein, Joel R.5; Burden, Angela7 |
| 刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
 |
| 出版日期 | 2014-06-01 |
| 卷号 | 441期号:1页码:24-62 |
| 关键词 | cosmological parameters cosmology: observations dark energy distance scale large-scale structure of Universe |
| 英文摘要 | 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. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000336249300002 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6580]  |
| 专题 | 国家天文台_星系宇宙学研究部 |
| 作者单位 | 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 |
| 推荐引用方式 GB/T 7714 | Anderson, Lauren,Aubourg, Eric,Bailey, Stephen,et al. The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2014,441(1):24-62. |
| APA | Anderson, Lauren.,Aubourg, Eric.,Bailey, Stephen.,Beutler, Florian.,Bhardwaj, Vaishali.,...&Zhao, Gong-Bo.(2014).The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,441(1),24-62. |
| MLA | Anderson, Lauren,et al."The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: baryon acoustic oscillations in the Data Releases 10 and 11 Galaxy samples".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 441.1(2014):24-62. |
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