The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space

被引：55

作者：

Zhao, Gong-Bo ^{[1
,2
]}

Wang, Yuting ^{[1
,2
]}

Saito, Shun ^{[3
,4
]}

Wang, Dandan ^{[1
]}

Ross, Ashley J. ^{[2
,5
]}

Beutler, Florian ^{[2
,6
]}

Grieb, Jan Niklas ^{[7
,8
]}

Chuang, Chia-Hsun ^{[9
,10
]}

Kitaura, Francisco-Shu ^{[10
]}

Rodriguez-Torres, Sergio ^{[11
,12
]}

Percival, Will J. ^{[2
]}

Brownstein, Joel R. ^{[13
]}

Cuesta, Antonio J. ^{[14
]}

Eisenstein, Daniel J. ^{[15
]}

Gil-Marin, Hector ^{[16
,17
]}

Kneib, Jean-Paul ^{[18
]}

Nichol, Robert C. ^{[2
]}

Olmstead, Matthew D. ^{[19
]}

Prada, Francisco

Rossi, Graziano ^{[20
]}

Salazar-Albornoz, Salvador ^{[21
,22
]}

Samushia, Lado ^{[2
]}

Sanchez, Ariel G. ^{[22
]}

Thomas, Daniel ^{[2
]}

Tinker, Jeremy L. ^{[23
]}

Tojeiro, Rita ^{[24
]}

Weinberg, David H. ^{[25
]}

Zhu, Fangzhou ^{[26
]}

机构：

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

[2] Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England

[3] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85740 Garching, Germany

[4] Univ Tokyo, Kavli Inst Phys & Math Univ IPMU, Kashiwa, Chiba 2778583, Japan

[5] Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43210 USA

[6] Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA

[7] Max Planck Inst Extraterr Phys, Postfach 1312, D-85741 Garching, Germany

[8] Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany

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

[10] Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany

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

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

[13] Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA

[14] Univ Barcelona IEEC UB, Inst Ciencies Cosmos ICCUB, Marti & Franques 1, E-08028 Barcelona, Spain

[15] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[16] Sorbonne Univ, ILP, 98 Bis Blvd Arago, F-75014 Paris, France

[17] Univ Paris 06, Lab Phys Nucl & Hautes Energies, 4 Pl Jussieu, F-75005 Paris, France

[18] Ecole Polytech Fed Lausanne, Observ Sauverny, Astrophys Lab, CH-1290 Versoix, Switzerland

[19] Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre 18711, PA USA

[20] Sejong Univ, Dept Astron & Space Sci, Seoul 143747, South Korea

[21] Ludwig Maximilians Univ Munchen, Univ Sternwarte, Scheinerstr 1, D-81679 Munich, Germany

[22] Max Planck Inst Extraterr Phys, Postfach 1312, D-85741 Garching, Germany

[23] NYU, Dept Phys, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA

[24] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland

[25] Ohio State Univ, Dept Astron, 140 West 18th Ave, Columbus, OH 43210 USA

[26] Yale Univ, Dept Phys, New Haven, CT 06511 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2017年 / 466卷 / 01期

基金：

美国国家科学基金会; 新加坡国家研究基金会;

关键词：

galaxies: distances and redshifts; cosmological parameters; cosmology: observations; dark energy; distance scale; large; scale structure of Universe; POWER-SPECTRUM ANALYSIS; ACOUSTIC-OSCILLATIONS; FINAL DATA; COSMOLOGICAL CONSEQUENCES; CMASS GALAXIES; DATA RELEASES; CONSTRAINTS; SCALE; BOSS; CONSTANT;

D O I：

10.1093/mnras/stw3199

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We perform a tomographic baryon acoustic oscillations (BAO) analysis using the monopole, quadrupole and hexadecapole of the redshift-space galaxy power spectrum measured from the pre-reconstructed combined galaxy sample of the completed Sloan Digital Sky Survey Baryon Oscillation Spectroscopic Survey (BOSS) Data Release12 covering the redshift range of 0.20 < z < 0.75. By allowing for overlap between neighbouring redshift slices, we successfully obtained the isotropic and anisotropic BAO distance measurements within nine redshift slices to a precision of 1.5-3.4 per cent for D-V/r(d), 1.8-4.2 per cent for DA/rd and 3.7-7.5 per cent for H-rd, depending on effective redshifts. We provide our BAO measurement of D-A/r(d) and Hrd with the full covariance matrix, which can be used for cosmological implications. Our measurements are consistent with those presented in Alam et al., in which the BAO distances are measured at three effective redshifts. We constrain dark energy parameters using our measurements and find an improvement of the Figure-of-Merit of dark energy in general due to the temporal BAO information resolved. This paper is a part of a set that analyses the final galaxy clustering data set from BOSS.

引用

页码：762 / 779

页数：18

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