The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range 0.8 &lt; z &lt; 2.2

doi:10.1093/mnras/sty453

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	The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range 0.8 < z < 2.2
	Gil-Marin, Hector 12,13; Guy, Julien 13,14; Zarrouk, Pauline 15; Burtin, Etienne 15; Chuang, Chia-Hsun 16,17,18; Percival, Will J.19; Ross, Ashley J.20; Ruggeri, Rossana 19; Tojerio, Rita 21; Zhao, Gong-Bo 19,22,23
刊名	MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
	2018-06-01
卷号	477 期号:2 页码:1591-1625
关键词	cosmological parameters large-scale structure of Universe
ISSN号	0035-8711
DOI	10.1093/mnras/sty453
英文摘要	We analyse the clustering of the Sloan Digital Sky Survey IV extended Baryon Oscillation Spectroscopic Survey Data Release 14 quasar sample (DR14Q). We measure the redshift space distortions using the power-spectrum monopole, quadrupole, and hexadecapole inferred from 148 659 quasars between redshifts 0.8 and 2.2, covering a total sky footprint of 2112.9 deg(2). We constrain the logarithmic growth of structure times the amplitude of dark matter density fluctuations, f sigma(8), and the Alcock-Paczynski dilation scales that allow constraints to be placed on the angular diameter distance D-A(z) and the Hubble H(z) parameter. At the effective redshift of z(eff) = 1.52, f sigma(8)(z(eff)) = 0.420 +/- 0.076, H(z(eff)) = [162 +/- 12] (r(s)(fid)/r(s)) kms(-1) Mpc(-1), and D-A(z(eff)) = [1.85 +/- 0.11] x 10(3) (r(s)/r(s)(fid)) Mpc, where rs is the comoving sound horizon at the baryon drag epoch and the superscript 'fid' stands for its fiducial value. The errors take into account the full error budget, including systematics and statistical contributions. These results are in full agreement with the current Lambda-Cold Dark Matter cosmological model inferred from Planck measurements. Finally, we compare our measurements with other eBOSS companion papers and find excellent agreement, demonstrating the consistency and complementarity of the different methods used for analysing the data.
资助项目	Labex ILP of the Idex SUPER[ANR-10-LABX-63] ; Agence Nationale de la Recherche of the programme Investissements d'avenir[ANR-11-IDEX-0004-02] ; 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 ; 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 ; Observatorio Naciona/MCTI ; Penn State University ; Shanghai Astronomical Observatory ; United Kingdom Participation Group ; University of Wisconsin ; Office of Science of the U.S. Department of Energy[DE-AC02-05CH11231] ; DOE Office of Science User Facility[DE-AC02-06CH11357]
WOS关键词	DIGITAL SKY SURVEY ; MOCK GALAXY CATALOGS ; DARK-MATTER HALOES ; SPACE DISTORTIONS ; ACOUSTIC-OSCILLATIONS ; FOURIER-SPACE ; MULTIPOLES ; RADIATION ; SYSTEM ; MODEL
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	OXFORD UNIV PRESS
WOS记录号	WOS:000434663200012
资助机构	Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; 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 ; 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 ; Observatorio Naciona/MCTI ; Observatorio Naciona/MCTI ; 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 ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; 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 ; 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 ; Observatorio Naciona/MCTI ; Observatorio Naciona/MCTI ; 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 ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; 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 ; 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 ; Observatorio Naciona/MCTI ; Observatorio Naciona/MCTI ; 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 ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Labex ILP of the Idex SUPER ; Labex ILP of the Idex SUPER ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; Agence Nationale de la Recherche of the programme Investissements d'avenir ; 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 ; 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 ; Observatorio Naciona/MCTI ; Observatorio Naciona/MCTI ; 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 ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; DOE Office of Science User Facility ; DOE Office of Science User Facility
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/21651]
专题	中国科学院国家天文台
通讯作者	Gil-Marin, Hector
作者单位	1.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China 2.Aix Marseille Univ, CNRS, LAM, 38 Rue F Joliot Curie, F-13388 Marseille 13, France 3.Leibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany 4.Hunbold Univ Berlin, Inst Phys, Newtonstrasse 15, D-12589 Berlin, Germany 5.Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA 6.Argonne Natl Lab, HEP, Lemont, IL 60439 USA 7.Argonne Natl Lab, MCS Div, Argonne, IL 60439 USA 8.Sejong Univ, Dept Astron & Space Sci, Seoul 143747, South Korea 9.Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA 10.Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
推荐引用方式 GB/T 7714	Gil-Marin, Hector,Guy, Julien,Zarrouk, Pauline,et al. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range 0.8 < z < 2.2[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,477(2):1591-1625.
APA	Gil-Marin, Hector.,Guy, Julien.,Zarrouk, Pauline.,Burtin, Etienne.,Chuang, Chia-Hsun.,...&Zhao, Cheng.(2018).The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range 0.8 < z < 2.2.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,477(2),1591-1625.
MLA	Gil-Marin, Hector,et al."The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: structure growth rate measurement from the anisotropic quasar power spectrum in the redshift range 0.8 < z < 2.2".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 477.2(2018):1591-1625.