The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering
文献类型:期刊论文
作者 | Chuang, Chia-Hsun1,2; Prada, Francisco1,3,4; Pellejero-Ibanez, Marcos5,6; Beutler, Florian7,8; Cuesta, Antonio J.9; Eisenstein, Daniel J.10; Escoffier, Stephanie11; Ho, Shirley12; Kitaura, Francisco-Shu2,7,13,14; Kneib, Jean-Paul15,16 |
刊名 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
出版日期 | 2016-10-01 |
卷号 | 461期号:4页码:3781-3793 |
关键词 | cosmological parameters cosmology: observations distance scale large-scale structure of Universe |
英文摘要 | With the largest spectroscopic galaxy survey volume drawn from the SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS), we can extract cosmological constraints from the measurements of redshift and geometric distortions at quasi-linear scales (e.g. above 50 h(-1) Mpc). We analyse the broad-range shape of the monopole and quadrupole correlation functions of the BOSS Data Release 12 (DR12) CMASS galaxy sample, at the effective redshift z = 0.59, to obtain constraints on the Hubble expansion rate H(z), the angular-diameter distance D-A(z), the normalized growth rate f(z)sigma(8)(z), and the physical matter density Omega(m)h(2). We obtain robust measurements by including a polynomial as the model for the systematic errors, and find it works very well against the systematic effects, e.g. ones induced by stars and seeing. We provide accurate measurements {D-A(0.59)r(s,fid)/r(s), H(0.59)r(s)/r(s, fid), f(0.59)sigma(8)(0.59), Omega(m)h(2)} = {1427 +/- 26 Mpc, 97.3 +/- 3.3 km s(-1) Mpc(-1), 0.488 +/- 0.060, 0.135 +/- 0.016}, where r(s) is the comoving sound horizon at the drag epoch and r(s, fid) = 147.66 Mpc is the sound scale of the fiducial cosmology used in this study. The parameters which are not well constrained by our galaxy clustering analysis are marginalized over with wide flat priors. Since no priors from other data sets, e.g. cosmic microwave background (CMB), are adopted and no dark energy models are assumed, our results from BOSS CMASS galaxy clustering alone may be combined with other data sets, i. e. CMB, SNe, lensing or other galaxy clustering data to constrain the parameters of a given cosmological model. The uncertainty on the dark energy equation of state parameter, w, from CMB+CMASS is about 8 per cent. The uncertainty on the curvature fraction, Omega(k), is 0.3 per cent. We do not find deviation from flat Lambda CDM. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | DIGITAL SKY SURVEY ; LUMINOUS RED GALAXIES ; REDSHIFT-SPACE DISTORTIONS ; DATA RELEASE 9 ; FINAL DATA RELEASE ; MEASURING D-A ; ACOUSTIC-OSCILLATIONS ; POWER-SPECTRUM ; DARK ENERGY ; GROWTH-RATE |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000383514900031 |
源URL | [http://ir.bao.ac.cn/handle/114a11/6779] |
专题 | 国家天文台_星系宇宙学研究部 |
作者单位 | 1.Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain 2.Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany 3.Campus Int Excellence UAM CSIC, E-28049 Madrid, Spain 4.Inst Astrofis Andalucia CSIC, Glorieta Astron, E-18080 Granada, Spain 5.Inst Astrofis Canarias, C Via Lactea S-N, E-38200 Tenerife, Spain 6.Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain 7.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA 8.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England 9.Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Marti & Franques 1, E-08028 Barcelona, Spain 10.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA |
推荐引用方式 GB/T 7714 | Chuang, Chia-Hsun,Prada, Francisco,Pellejero-Ibanez, Marcos,et al. The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2016,461(4):3781-3793. |
APA | Chuang, Chia-Hsun.,Prada, Francisco.,Pellejero-Ibanez, Marcos.,Beutler, Florian.,Cuesta, Antonio J..,...&Thomas, Daniel.(2016).The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,461(4),3781-3793. |
MLA | Chuang, Chia-Hsun,et al."The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements from CMASS anisotropic galaxy clustering".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 461.4(2016):3781-3793. |
入库方式: OAI收割
来源:国家天文台
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