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The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications
Salazar-Albornoz, Salvador1,2; Sanchez, Ariel G.2; Grieb, Jan Niklas1,2; Crocce, Martin3; Scoccimarro, Roman4; Alam, Shadab5,6; Beutler, Florian7; Brownstein, Joel R.8; Chuang, Chia-Hsun10; Kitaura, Francisco-Shu; Olmstead, Matthew D.11; Percival, Will J.7; Prada, Francisco10,12,13; Rodriguez-Torres, Sergio10,12,14; Samushia, Lado7,15,16; Tinker, Jeremy4; Thomas, Daniel7; Tojeiro, Rita17; Wang, Yuting7,18; Zhao, Gong-bo18
2017-07-01
发表期刊MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷号468期号:3页码:2938-2956
摘要We investigate the cosmological implications of studying galaxy clustering using a tomographic approach applied to the final Baryon Oscillation Spectroscopic Survey (BOSS) DR12 galaxy sample, including both auto-and cross-correlation functions between redshift shells. We model the signal of the full shape of the angular correlation function, omega(theta), in redshift bins using state-of-the-art modelling of non-linearities, bias and redshift-space distortions. We present results on the redshift evolution of the linear bias of BOSS galaxies, which cannot be obtained with traditional methods for galaxy-clustering analysis. We also obtain constraints on cosmological parameters, combining this tomographic analysis with measurements of the cosmic microwave background (CMB) and Type Ia supernova (SNIa). We explore a number of cosmological models, including the standard Lambda cold dark matter model and its most interesting extensions, such as deviations from omega(DE) =-1, non-minimal neutrino masses, spatial curvature and deviations from general relativity (GR) using the growth-index gamma parametrization. These results are, in general, comparable to the most precise present-day constraints on cosmological parameters, and show very good agreement with the standard model. In particular, combining CMB, omega(theta) and SNIa, we find a value of w(DE) consistent with -1 to a precision better than 5 per cent when it is assumed to be constant in time, and better than 6 per cent when we also allow for a spatially curved Universe.
文章类型Article
关键词Cosmological Parameters Large-scale Structure Of Universe
WOS标题词Science & Technology ; Physical Sciences
资助者Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; 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 ; ESA ; NASA ; NASA ; Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; 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 ; ESA ; NASA ; NASA
DOI10.1093/mnras/stx633
关键词[WOS]DIGITAL SKY SURVEY ; SUPERNOVA LEGACY SURVEY ; LUMINOUS RED GALAXIES ; DARK-ENERGY ; ACOUSTIC-OSCILLATIONS ; FOURIER SPACE ; DATA RELEASE ; FINAL DATA ; SYSTEMATIC UNCERTAINTIES ; PARAMETER CONSTRAINTS
收录类别SCI
语种英语
资助者Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; 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 ; ESA ; NASA ; NASA ; Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; Trans-regional Collaborative Research Centre TRR33 The Dark Universe of the Deutsche Forgschungsgemeinschaft (DFG) ; 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 ; ESA ; NASA ; NASA
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000402808700036
引用统计
被引频次:6[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.bao.ac.cn/handle/114a11/8801
专题星系宇宙学研究部
作者单位1.Ludwig Maximilians Univ Munchen, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany
2.Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85741 Garching, Germany
3.IEEC CSIC, Inst Ciencies Espai, Campus UAB,Carrer Can Magrans,S-N, E-08193 Barcelona, Spain
4.NYU, Dept Phys, Ctr Cosmol & Particle Phys, 4 Washington Pl, New York, NY 10003 USA
5.Carnegie Mellon Univ, Dept Phys, 500 Forbes Ave, Pittsburgh, PA 15213 USA
6.Carnegie Mellon Univ, McWilliams Ctr Cosmol, 500 Forbes Ave, Pittsburgh, PA 15213 USA
7.Univ Protsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
8.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
9.Leibniz Inst Astrophys AIP, Sternwarte 16, D-14482 Potsdam, Germany
10.Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain
11.Kings Coll, Dept Chem & Phys, 133 North River St, Wilkes Barre, PA 18711 USA
12.Univ Autonoma Madrid, Dept Fis Teor, E-28049 Madrid, Spain
13.Inst Astrofis Andalucia CSIC, Glorieta Astron, E-18080 Granada, Spain
14.Campus Int Excellence UAM CSIC, E-28049 Madrid, Spain
15.Kansas State Univ, Manhattan, KS 66506 USA
16.Ilia State Univ, Natl Abastumani Astrophys Observ, 2A Kazbegi Ave, GE-1060 Tbilisi, Rep of Georgia
17.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
18.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
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Salazar-Albornoz, Salvador,Sanchez, Ariel G.,Grieb, Jan Niklas,et al. The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2017,468(3):2938-2956.
APA Salazar-Albornoz, Salvador.,Sanchez, Ariel G..,Grieb, Jan Niklas.,Crocce, Martin.,Scoccimarro, Roman.,...&Zhao, Gong-bo.(2017).The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,468(3),2938-2956.
MLA Salazar-Albornoz, Salvador,et al."The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: angular clustering tomography and its cosmological implications".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 468.3(2017):2938-2956.
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