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The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2

文献类型：期刊论文

作者Zarrouk, Pauline1; Burtin, Etienne1; Gil-Marin, Hector2,3; Ross, Ashley J.4,5; Tojeiro, Rita6; Paris, Isabelle7; Dawson, Kyle S.8; Myers, Adam D.8; Percival, Will J.5; Chuang, Chia-Hsun9,10,11
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2018-06-01
卷号477期号:2页码:1626-1650
ISSN号0035-8711
关键词cosmological parameters cosmology: observations dark energy large-scale structure of Universe
DOI10.1093/mnras/sty506
英文摘要We present the clustering measurements of quasars in configuration space based on the Data Release 14 (DR14) of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey (eBOSS). This data set includes 148 659 quasars spread over the redshift range 0.8 <= z <= 2.2 and spanning 2112.9 deg(2). We use the Convolution Lagrangian Perturbation Theory approach with a Gaussian Streaming model for the redshift space distortions of the correlation function and demonstrate its applicability for dark matter haloes hosting eBOSS quasar tracers. At the effective redshift z(eff) = 1.52, we measure the linear growth rate of structure f sigma(8)(z(eff)) = 0.426 +/- 0.077, the expansion rate H(z(eff)) = 159(-13)(+12)(r(s)(fid)/r(s)) kms(-1)Mpc(-1), and the angular diameter distance D-A(z(eff)) = 1850(-115)(+90) (r(s)/r(s)(fid)) Mpc, where r(s) is the sound horizon at the end of the baryon drag epoch and r(s)(fid) is its value in the fiducial cosmology. The quoted uncertainties include both systematic and statistical contributions. The results on the evolution of distances are consistent with the predictions of flat Lambda-cold dark matter cosmology with Planck parameters, and the measurement of f sigma(8) extends the validity of General Relativity to higher redshifts (z > 1). This paper is released with companion papers using the same sample. The results on the cosmological parameters of the studies are found to be in very good agreement, providing clear evidence of the complementarity and of the robustness of the first full-shape clustering measurements with the eBOSS DR14 quasar sample.
WOS关键词DIGITAL SKY SURVEY ; POWER-SPECTRUM ANALYSIS ; DARK-MATTER HALOES ; SPACE DISTORTIONS ; ACOUSTIC-OSCILLATIONS ; COSMOLOGICAL CONSTANT ; PERTURBATION-THEORY ; LINEAR REGIME ; ENERGY SURVEY ; 2DF-SDSS LRG
资助项目P2IO LabEx[ANR-10-LABX-0038] ; Labex ILP of the Idex SUPER[ANR-10-LABX-63] ; Agence Nationalede la Recherche[ANR-11-IDEX-0004-02] ; Ohio State University Center for Cosmology and ParticlePhysics ; NSFC[1171001024] ; NSFC[11673025] ; Royal Society Newton Advanced Fellowship ; U.S. Department of Energy[DE-AC02-06CH11357] ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)[2017077508] ; faculty research fund of Sejong University ; Alfred P. Sloan Foundation ; National Science Foundation ; U.S. Department of Energy Office of Science ; University of Arizona ; Brazilian Participation Group ; Brookhaven National Laboratory ; Carnegie Mellon University ; University of Florida ; French Participation Group ; German Participation Group ; Harvard University ; Instituto de Astrofisica de Canarias ; Michigan State/Notre Dame/JINA Participation Group ; Johns Hopkins University ; Lawrence Berkeley National Laboratory ; Max Planck Institute for Astrophysics ; Max Planck Institute for Extraterrestrial Physics ; New Mexico State University ; New York University ; Ohio State University ; Pennsylvania State University ; University of Portsmouth ; Princeton University ; Spanish Participation Group ; University of Tokyo ; University of Utah ; Vanderbilt University ; University of Virginia ; University of Washington ; Yale University ; CarnegieMellon University ; Colorado University ; Boulder ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; National Astronomical Observatories of China ; Penn State University ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; University of Wisconsin ; DOE Office of Science User Facility[DE-AC02-06CH11357] ; ICG ; SEPNet ; Office of Science of the U.S. Department of Energy[DE-AC02-05CH11231]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000434663200013
资助机构P2IO LabEx ; P2IO LabEx ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationalede la Recherche ; Agence Nationalede la Recherche ; Ohio State University Center for Cosmology and ParticlePhysics ; Ohio State University Center for Cosmology and ParticlePhysics ; NSFC ; NSFC ; Royal Society Newton Advanced Fellowship ; Royal Society Newton Advanced Fellowship ; U.S. Department of Energy ; U.S. Department of Energy ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; 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 ; 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 ; CarnegieMellon University ; CarnegieMellon University ; Colorado University ; Colorado University ; Boulder ; Boulder ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; Penn State University ; Penn State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; University of Wisconsin ; University of Wisconsin ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; ICG ; ICG ; SEPNet ; SEPNet ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; P2IO LabEx ; P2IO LabEx ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationalede la Recherche ; Agence Nationalede la Recherche ; Ohio State University Center for Cosmology and ParticlePhysics ; Ohio State University Center for Cosmology and ParticlePhysics ; NSFC ; NSFC ; Royal Society Newton Advanced Fellowship ; Royal Society Newton Advanced Fellowship ; U.S. Department of Energy ; U.S. Department of Energy ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; 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 ; 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 ; CarnegieMellon University ; CarnegieMellon University ; Colorado University ; Colorado University ; Boulder ; Boulder ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; Penn State University ; Penn State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; University of Wisconsin ; University of Wisconsin ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; ICG ; ICG ; SEPNet ; SEPNet ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; P2IO LabEx ; P2IO LabEx ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationalede la Recherche ; Agence Nationalede la Recherche ; Ohio State University Center for Cosmology and ParticlePhysics ; Ohio State University Center for Cosmology and ParticlePhysics ; NSFC ; NSFC ; Royal Society Newton Advanced Fellowship ; Royal Society Newton Advanced Fellowship ; U.S. Department of Energy ; U.S. Department of Energy ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; 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 ; 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 ; CarnegieMellon University ; CarnegieMellon University ; Colorado University ; Colorado University ; Boulder ; Boulder ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; Penn State University ; Penn State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; University of Wisconsin ; University of Wisconsin ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; ICG ; ICG ; SEPNet ; SEPNet ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; P2IO LabEx ; P2IO LabEx ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationalede la Recherche ; Agence Nationalede la Recherche ; Ohio State University Center for Cosmology and ParticlePhysics ; Ohio State University Center for Cosmology and ParticlePhysics ; NSFC ; NSFC ; Royal Society Newton Advanced Fellowship ; Royal Society Newton Advanced Fellowship ; U.S. Department of Energy ; U.S. Department of Energy ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST) ; faculty research fund of Sejong University ; faculty research fund of Sejong University ; 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 ; 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 ; CarnegieMellon University ; CarnegieMellon University ; Colorado University ; Colorado University ; Boulder ; Boulder ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Harvard-Smithsonian Center for Astrophysics Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Kavli Institute for the Physics and Mathematics of the Universe Max-Planck-Institut fuer Astrophysik (MPA Garching) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; Penn State University ; Penn State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; University of Wisconsin ; University of Wisconsin ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; ICG ; ICG ; SEPNet ; SEPNet ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy
源URL[http://ir.bao.ac.cn/handle/114a11/21714]  
专题中国科学院国家天文台
通讯作者Zarrouk, Pauline; Burtin, Etienne
作者单位1.Univ ParisSaclay, IRFU, CLA, F-91191 Gif Sur Yvette, France
2.Sorbonne Univ, ILP, 98 Bis Blvd Arago, F-75014 Paris, France
3.Univ Paris 06, Lab Phys Nucl & Hawes Energies, 4 Pl Jussieu, F-75005 Paris, France
4.Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
5.Univ Portsmouth, Inst Cosmol & Gravitat, DennisSciama Bldg, Portsmouth POI 3EX, Hants, England
6.Univ St Andrews, Sch Phys & Astron, St Andrews KY16 95S, Fife, Scotland
7.Aix Marseille Univ, CNRS, LAM, 38 Rue Joliot Curie, F-13388 Marseille 13, France
8.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
9.Leibniz Inst Astrophys Potsdam AIP, Stemwarte 16, D-14482 Potsdam, Germany
10.Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
推荐引用方式
GB/T 7714		 Zarrouk, Pauline,Burtin, Etienne,Gil-Marin, Hector,et al. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,477(2):1626-1650.
APA Zarrouk, Pauline.,Burtin, Etienne.,Gil-Marin, Hector.,Ross, Ashley J..,Tojeiro, Rita.,...&Zhao, Cheng.(2018).The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,477(2),1626-1650.
MLA Zarrouk, Pauline,et al."The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 477.2(2018):1626-1650.

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