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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample

文献类型：期刊论文

作者McBride, Cameron K.15; Malanushenko, Viktor6; Malanushenko, Elena6; Kitaura, Francisco4,5,21; Kirkby, David22; Kinemuchi, Karen6; Ho, Shirley2,3; Hand, Nick21; Grieb, Jan Niklas19,20; Gil-Marin, Hector17,18
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2017-09-01
卷号470期号:3页码:2617-2652
关键词Distance Scale Large-scale Structure Of Universe Cosmology: Observations
DOI10.1093/mnras/stx721
文献子类Article
英文摘要We present cosmological results from the final galaxy clustering data set of the Baryon Oscillation Spectroscopic Survey, part of the Sloan Digital Sky Survey III. Our combined galaxy sample comprises 1.2 million massive galaxies over an effective area of 9329 deg(2) and volume of 18.7 Gpc(3), divided into three partially overlapping redshift slices centred at effective redshifts 0.38, 0.51 and 0.61. We measure the angular diameter distance DM and Hubble parameter H from the baryon acoustic oscillation (BAO) method, in combination with a cosmic microwave background prior on the sound horizon scale, after applying reconstruction to reduce non-linear effects on the BAO feature. Using the anisotropic clustering of the pre-reconstruction density field, we measure the product DMH from the Alcock-Paczynski (AP) effect and the growth of structure, quantified by f sigma(8(z)), from redshift-space distortions (RSD). We combine individual measurements presented in seven companion papers into a set of consensus values and likelihoods, obtaining constraints that are tighter and more robust than those from any one method; in particular, the AP measurement from sub-BAO scales sharpens constraints from post-reconstruction BAOs by breaking degeneracy between D-M and H. Combined with Planck 2016 cosmic microwave background measurements, our distance scale measurements simultaneously imply curvature Omega(K) = 0.0003 +/- 0.0026 and a dark energy equation-of-state parameter w = -1.01 +/- 0.06, in strong affirmation of the spatially flat cold dark matter (CDM) model with a cosmological constant (Lambda CDM). Our RSD measurements of f sigma(8), at 6 per cent precision, are similarly consistent with this model. When combined with supernova Ia data, we find H-0 = 67.3 +/- 1.0 km s(-1) Mpc(-1) even for our most general dark energy model, in tension with some direct measurements. Adding extra relativistic species as a degree of freedom loosens the constraint only slightly, to H-0 = 67.8 +/- 1.2 km s(-1) Mpc(-1). Assuming flat Lambda CDM, we find Omega(m) = 0.310 +/- 0.005 and H-0 = 67.6 +/- 0.5 km s(-1) Mpc(-1), and we find a 95 per cent upper limit of 0.16 eV c(-2) on the neutrino mass sum.
WOS关键词DIGITAL SKY SURVEY ; REDSHIFT-SPACE DISTORTIONS ; LUMINOUS RED GALAXIES ; PROBING DARK ENERGY ; POWER-SPECTRUM ANALYSIS ; LARGE-SCALE STRUCTURE ; SURVEY IMAGING DATA ; MEASURING D-A ; ACOUSTIC-OSCILLATIONS ; DATA RELEASE
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000406844800008
资助机构Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation (DFG)(TR33) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation (DFG)(TR33) ; UK Space Agency(ST/N00180X/1) ; UK Space Agency(ST/N00180X/1) ; U.S. Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0010331) ; U.S. Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0010331) ; European Research Council under the European Community(FP7-IDEAS-Phys. LSS 240117) ; European Research Council under the European Community(FP7-IDEAS-Phys. LSS 240117) ; Spanish MINECO of ICCUB (Unidad de Excelencia 'Maria de Maeztu')(AYA2014-58747-P ; Spanish MINECO of ICCUB (Unidad de Excelencia 'Maria de Maeztu')(AYA2014-58747-P ; U.S. Department ofEnergy, Office of Science, Office of High Energy Physics(DE-SC0013718 ; U.S. Department ofEnergy, Office of Science, Office of High Energy Physics(DE-SC0013718 ; Labex ILP part of the Idex SUPER(ANR-10-LABX-63) ; Labex ILP part of the Idex SUPER(ANR-10-LABX-63) ; Agence Nationale de la Recherche, as part of the programme Investissements d'avenir(ANR-11-IDEX-0004-02) ; Agence Nationale de la Recherche, as part of the programme Investissements d'avenir(ANR-11-IDEX-0004-02) ; UK Science and Technology Facilities Research Council(ST/M001709/1 ; UK Science and Technology Facilities Research Council(ST/M001709/1 ; European Research Council(614030 Darksurvey) ; European Research Council(614030 Darksurvey) ; STFC ; STFC ; Ernest Rutherford Fellowship scheme ; Ernest Rutherford Fellowship scheme ; 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) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; DOE(DE-AC02-98CH10886) ; DOE(DE-AC02-98CH10886) ; Science and Technology Facilities Council via an Ernest Rutherford Fellowship(ST/K004719/1) ; Science and Technology Facilities Council via an Ernest Rutherford Fellowship(ST/K004719/1) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; 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 and Canada ; NASA and Canada ; Office of Science of the U.S. Department of Energy(DE-AC02-05CH11231) ; Office of Science of the U.S. Department of Energy(DE-AC02-05CH11231) ; MDM-2014-0369) ; MDM-2014-0369) ; DE-SC0009959 ; DE-SC0009959 ; ST/N000668/1) ; ST/N000668/1) ; DE-SC0014329) ; DE-SC0014329) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation (DFG)(TR33) ; Trans-regional Collaborative Research Centre 'The Dark Universe' of the German Research Foundation (DFG)(TR33) ; UK Space Agency(ST/N00180X/1) ; UK Space Agency(ST/N00180X/1) ; U.S. Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0010331) ; U.S. Department of Energy, Office of Science, Office of High Energy Physics(DE-SC0010331) ; European Research Council under the European Community(FP7-IDEAS-Phys. LSS 240117) ; European Research Council under the European Community(FP7-IDEAS-Phys. LSS 240117) ; Spanish MINECO of ICCUB (Unidad de Excelencia 'Maria de Maeztu')(AYA2014-58747-P ; Spanish MINECO of ICCUB (Unidad de Excelencia 'Maria de Maeztu')(AYA2014-58747-P ; U.S. Department ofEnergy, Office of Science, Office of High Energy Physics(DE-SC0013718 ; U.S. Department ofEnergy, Office of Science, Office of High Energy Physics(DE-SC0013718 ; Labex ILP part of the Idex SUPER(ANR-10-LABX-63) ; Labex ILP part of the Idex SUPER(ANR-10-LABX-63) ; Agence Nationale de la Recherche, as part of the programme Investissements d'avenir(ANR-11-IDEX-0004-02) ; Agence Nationale de la Recherche, as part of the programme Investissements d'avenir(ANR-11-IDEX-0004-02) ; UK Science and Technology Facilities Research Council(ST/M001709/1 ; UK Science and Technology Facilities Research Council(ST/M001709/1 ; European Research Council(614030 Darksurvey) ; European Research Council(614030 Darksurvey) ; STFC ; STFC ; Ernest Rutherford Fellowship scheme ; Ernest Rutherford Fellowship scheme ; 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) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; DOE(DE-AC02-98CH10886) ; DOE(DE-AC02-98CH10886) ; Science and Technology Facilities Council via an Ernest Rutherford Fellowship(ST/K004719/1) ; Science and Technology Facilities Council via an Ernest Rutherford Fellowship(ST/K004719/1) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; U.S. Department of Energy Office of Science ; 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 and Canada ; NASA and Canada ; Office of Science of the U.S. Department of Energy(DE-AC02-05CH11231) ; Office of Science of the U.S. Department of Energy(DE-AC02-05CH11231) ; MDM-2014-0369) ; MDM-2014-0369) ; DE-SC0009959 ; DE-SC0009959 ; ST/N000668/1) ; ST/N000668/1) ; DE-SC0014329) ; DE-SC0014329)
源URL[http://ir.bao.ac.cn/handle/114a11/20072]  
专题国家天文台_星系宇宙学研究部
作者单位1.Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway
2.Carnegie Mellon Univ, Dept Phys, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
3.Carnegie Mellon Univ, McWilliams Ctr Cosmol, 5000 Forbes Ave, Pittsburgh, PA 15213 USA
4.Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany
5.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
6.New Mexico State Univ, Apache Point Observ, POB 59, Sunspot, NM 88349 USA
7.Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Univ Ski Pr 13, Moscow 119992, Russia
8.Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
9.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
10.Natl Opt Astron Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA
推荐引用方式
GB/T 7714		 McBride, Cameron K.,Malanushenko, Viktor,Malanushenko, Elena,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,470(3):2617-2652.
APA McBride, Cameron K..,Malanushenko, Viktor.,Malanushenko, Elena.,Kitaura, Francisco.,Kirkby, David.,...&Bailey, Stephen.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,470(3),2617-2652.
MLA McBride, Cameron K.,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 470.3(2017):2617-2652.

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来源：国家天文台

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