NAOC Open IR  > 星系宇宙学研究部
The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
Zhao, Gong-Bo1,2; Wang, Yuting1,2; Saito, Shun3,4; Wang, Dandan1; Ross, Ashley J.2,5; Beutler, Florian2,6; Grieb, Jan Niklas7,8; Chuang, Chia-Hsun9,10; Kitaura, Francisco-Shu10; Rodriguez-Torres, Sergio11,12; Percival, Will J.2; Brownstein, Joel R.13; Cuesta, Antonio J.14; Eisenstein, Daniel J.15; Gil-Marin, Hector16,17; Kneib, Jean-Paul18; Nichol, Robert C.2; Olmstead, Matthew D.19; Prada, Francisco; Rossi, Graziano20; Salazar-Albornoz, Salvador21,22; Samushia, Lado2; Sanchez, Ariel G.22; Thomas, Daniel2; Tinker, Jeremy L.23; Tojeiro, Rita24; Weinberg, David H.25; Zhu, Fangzhou26
2017-04-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume466Issue:1Pages:762-779
AbstractWe 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.
SubtypeArticle
KeywordGalaxies: Distances And Redshifts Cosmological Parameters Cosmology: Observations Dark Energy Distance Scale Large Scale Structure Of Universe
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationStrategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; University of Portsmouth ; University of Portsmouth ; 1000 Young Talents program in China ; 1000 Young Talents program in China ; NSFC(11403034) ; NSFC(11403034) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; Participating Institutions ; Participating Institutions ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; NAOC ; NAOC ; Strategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; University of Portsmouth ; University of Portsmouth ; 1000 Young Talents program in China ; 1000 Young Talents program in China ; NSFC(11403034) ; NSFC(11403034) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; Participating Institutions ; Participating Institutions ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; NAOC ; NAOC
DOI10.1093/mnras/stw3199
WOS KeywordDIGITAL SKY SURVEY ; POWER-SPECTRUM ANALYSIS ; FINAL DATA RELEASE ; ACOUSTIC-OSCILLATIONS ; COSMOLOGICAL CONSTANT ; DARK ENERGY ; COSMIC ACCELERATION ; REDSHIFT SURVEYS ; CMASS GALAXIES ; SCALE
Indexed BySCI
Language英语
Funding OrganizationStrategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; University of Portsmouth ; University of Portsmouth ; 1000 Young Talents program in China ; 1000 Young Talents program in China ; NSFC(11403034) ; NSFC(11403034) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; Participating Institutions ; Participating Institutions ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; NAOC ; NAOC ; Strategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; Strategic Priority Research Program 'The Emergence of Cosmological Structures' of the Chinese Academy of Sciences(XDB09000000) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; National Astronomical Observatories, Chinese Academy of Sciences (NAOC) ; University of Portsmouth ; University of Portsmouth ; 1000 Young Talents program in China ; 1000 Young Talents program in China ; NSFC(11403034) ; NSFC(11403034) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; National Research Foundation of Korea (NRF) through NRF-SGER -Korean Ministry of Education, Science and Technology (MoEST)(2014055950) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; Participating Institutions ; Participating Institutions ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; Office of Science of the U.S. Department of Energy(DEAC02-05CH11231) ; NAOC ; NAOC
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000398112400052
Citation statistics
Cited Times:29[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8223
Collection星系宇宙学研究部
Affiliation1.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
Recommended Citation
GB/T 7714
Zhao, Gong-Bo,Wang, Yuting,Saito, Shun,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,466(1):762-779.
APA Zhao, Gong-Bo.,Wang, Yuting.,Saito, Shun.,Wang, Dandan.,Ross, Ashley J..,...&Zhu, Fangzhou.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,466(1),762-779.
MLA Zhao, Gong-Bo,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 466.1(2017):762-779.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Zhao, Gong-Bo]'s Articles
[Wang, Yuting]'s Articles
[Saito, Shun]'s Articles
Baidu academic
Similar articles in Baidu academic
[Zhao, Gong-Bo]'s Articles
[Wang, Yuting]'s Articles
[Saito, Shun]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Zhao, Gong-Bo]'s Articles
[Wang, Yuting]'s Articles
[Saito, Shun]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.