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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges
Sanchez, Ariel G.1; Scoccimarro, Roman2; Crocce, Martin3; Grieb, Jan Niklas1,4; Salazar-Albornoz, Salvador1,4; Dalla Vecchia, Claudio5,6; Lippich, Martha1,4; Beutler, Florian7,8; Brownstein, Joel R.9; Chuang, Chia-Hsun10,11; Eisenstein, Daniel J.12; Kitaura, Francisco-Shu8,11,13,14; Olmstead, Matthew D.15; Percival, Will J.7; Prada, Francisco10,16,17; Rodriguez-Torres, Sergio10,16,18; Ross, Ashley J.7,19; Samushia, Lado7,20,21; Seo, Hee-Jong22; Tinker, Jeremy2; Tojeiro, Rita23; Vargas-Magana, Mariana24,25,26; Wang, Yuting7,27; Zhao, Gong-Bo7,27
2017
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume464Issue:2Pages:1640-1658
AbstractWe explore the cosmological implications of anisotropic clustering measurements in configuration space of the final galaxy samples from Data Release 12 of the Sloan Digital Sky Survey III Baryon Oscillation Spectroscopic Survey. We implement a new detailed modelling of the effects of non-linearities, bias and redshift-space distortions that can be used to extract unbiased cosmological information from our measurements for scales s greater than or similar to 20 h(-1) Mpc. We combined the information from Baryon Oscillation Spectroscopic Survey (BOSS) with the latest cosmic microwave background (CMB) observations and Type Ia supernovae samples and found no significant evidence for a deviation from the Lambda cold dark matter (Lambda CDM) cosmological model. In particular, these data sets can constrain the dark energy equation-of-state parameter to w(DE) = -0.996 +/- 0.042 when to be assumed time independent, the curvature of the Universe to Omega(k) = -0.0007 +/- 0.0030 and the sum of the neutrino masses to Sigma m nu < 0.25 eV at 95 per cent confidence levels. We explore the constraints on the growth rate of cosmic structures assuming f(z)=Omega(m)(z)(gamma) and obtain gamma = 0.609 +/- 0.079, in good agreement with the predictions of general relativity of gamma=0.55. We compress the information of our clustering measurements into constraints on the parameter combinations D-V(z)/r(d), F-AP(z) and f sigma(8)(z) at z(eff) = 0.38, 0.51 and 0.61 with their respective covariance matrices and find good agreement with the predictions for these parameters obtained from the best-fitting Lambda CDM model to the CMB data from the Planck satellite. This paper is part of a set that analyses the final galaxy clustering data set from BOSS. The measurements and likelihoods presented here are combined with others by Alam et al. to produce the final cosmological constraints from BOSS.
SubtypeArticle
KeywordCosmological Parameters Large-scale Structure Of Universe
WOS HeadingsScience & Technology ; Physical Sciences
Funding OrganizationTrans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; NSF(AST-1109432) ; NSF(AST-1109432) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy ; US Department of Energy ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; University of Cambridge ; University of Cambridge ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; ESA Member States ; ESA Member States ; NASA ; NASA ; SEV-2015-0548 ; SEV-2015-0548 ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; NSF(AST-1109432) ; NSF(AST-1109432) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy ; US Department of Energy ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; University of Cambridge ; University of Cambridge ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; ESA Member States ; ESA Member States ; NASA ; NASA ; SEV-2015-0548 ; SEV-2015-0548 ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308)
DOI10.1093/mnras/stw2443
WOS KeywordDIGITAL SKY SURVEY ; MICROWAVE BACKGROUND ANISOTROPIES ; POWER-SPECTRUM ANALYSIS ; LUMINOUS RED GALAXIES ; REDSHIFT-SPACE ; DATA RELEASE ; ACOUSTIC-OSCILLATIONS ; DARK ENERGY ; FINAL DATA ; PARAMETER CONSTRAINTS
Indexed BySCI
Language英语
Funding OrganizationTrans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; NSF(AST-1109432) ; NSF(AST-1109432) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy ; US Department of Energy ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; University of Cambridge ; University of Cambridge ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; ESA Member States ; ESA Member States ; NASA ; NASA ; SEV-2015-0548 ; SEV-2015-0548 ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation(TR33) ; NSF(AST-1109432) ; NSF(AST-1109432) ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Spanish Ministry of Economy and Competitiveness (MINECO)(SEV-2011-0187 ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Programa de Apoyo a Proyectos de Investigacion e Innovacion Tecnologica (PAPITT)(IA102516) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; US Department of Energy ; US Department of Energy ; University of Arizona ; University of Arizona ; Brazilian Participation Group ; Brazilian Participation Group ; Brookhaven National Laboratory ; Brookhaven National Laboratory ; University of Cambridge ; University of Cambridge ; Carnegie Mellon University ; Carnegie Mellon University ; University of Florida ; University of Florida ; French Participation Group ; French Participation Group ; German Participation Group ; German Participation Group ; Harvard University ; Harvard University ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; Ohio State University ; Ohio State University ; Pennsylvania State University ; Pennsylvania State University ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; Vanderbilt University ; Vanderbilt University ; University of Virginia ; University of Virginia ; University of Washington ; University of Washington ; Yale University ; Yale University ; ESA Member States ; ESA Member States ; NASA ; NASA ; SEV-2015-0548 ; SEV-2015-0548 ; AYA2013-46886 ; AYA2013-46886 ; AYA2014-58308) ; AYA2014-58308)
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000393647100028
Citation statistics
Cited Times:33[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/8277
Collection星系宇宙学研究部
Affiliation1.Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85741 Garching, Germany
2.NYU, Dept Phys, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA
3.CSIC, IEEC, Inst Ciencies Espai, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain
4.Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
5.Inst Astrofis Canarias, C Via Lactea S-N, E-38205 Tenerife, Spain
6.Univ La Laguna, Dept Astrofis, Ave Astrofis Francisco Saanchez S-N, E-38206 Tenerife, Spain
7.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
8.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
9.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
10.Univ Autonoma Madrid, Inst Fis Teor, CSIC, E-28049 Madrid, Spain
11.Leibniz Inst Astrophys Potsdam, Sternwarte 16, D-14482 Potsdam, Germany
12.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
13.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
14.Univ Calif Berkeley, Dept Astron, 601 Campbell Hall, Berkeley, CA 94720 USA
15.Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre, PA 18711 USA
16.Campus Int Excellence UAM CSIC, E-28049 Madrid, Spain
17.CSIC, Inst Astrofis Andalucia, Glorieta Astron, E-18080 Granada, Spain
18.Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
19.Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
20.Kansas State Univ, Manhattan, KS 66506 USA
21.Ilia State Univ, Natl Abastumani Astrophys Observ, 2A Kazbegi Ave, GE-1060 Tbilisi, Rep of Georgia
22.Ohio Univ, Dept Phys & Astron, 251B Clippinger Labs, Athens, OH 45701 USA
23.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
24.Univ Nacl Autonoma Mexico, Inst Fis, Apdo Postal 20-364, Mexico City 01000, DF, Mexico
25.Carnegie Mellon Univ, Dept Phys, 5000 Forbes Ave, Pittsburgh, PA 15217 USA
26.Carnegie Mellon Univ, McWilliams Ctr Cosmol, 5000 Forbes Ave, Pittsburgh, PA 15217 USA
27.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Sanchez, Ariel G.,Scoccimarro, Roman,Crocce, Martin,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,464(2):1640-1658.
APA Sanchez, Ariel G..,Scoccimarro, Roman.,Crocce, Martin.,Grieb, Jan Niklas.,Salazar-Albornoz, Salvador.,...&Zhao, Gong-Bo.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,464(2),1640-1658.
MLA Sanchez, Ariel G.,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Cosmological implications of the configuration-space clustering wedges".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 464.2(2017):1640-1658.
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