中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift-space distortions between redshift 0.8 and 2.2

文献类型:期刊论文

作者Ruggeri, Rossana2; Percival, Will J.2; Gil-Marin, Hector3,4; Beutler, Florian2,5; Mueller, Eva-Maria2; Zhu, Fangzhou6; Padmanabhan, Nikhil6; Zhao, Gong-Bo2,7; Zarrouk, Pauline8; Sanchez, Ariel G.9
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2019-03-01
卷号483期号:3页码:3878-3887
ISSN号0035-8711
关键词cosmology: observations dark energy dark matter large-scale structure of Universe
DOI10.1093/mnras/sty3395
英文摘要We measure the growth rate and its evolution using the anisotropic clustering of the extended Baryon Oscillation Spectroscopic Survey (eBOSS) Data Release 14 (DR14) quasar sample, which includes 148 659 quasars covering the wide redshift range of 0.8 < z < 2.2 and a sky area of 2112.90 deg(2). To optimize measurements we deploy a redshift-dependent weighting scheme, which allows us to avoid binning and perform the data analysis consistently including the redshift evolution across the sample. We perform the analysis in Fourier space, and use the redshift evolving power spectrum multipoles to measure the redshift-space distortion parameter f sigma(8) and parameters controlling the anisotropic projection of the cosmological perturbations. We measure f sigma(8)(z = 1.52) = 0.43 +/- 0.05 and df sigma(8)/dz (z = 1.52) = -0.16 +/- 0.08, consistent with the expectation for a lambda cold dark matter cosmology as constrained by the Planck experiment.
WOS关键词POWER-SPECTRUM ; ACOUSTIC-OSCILLATIONS ; GALAXIES
资助项目European Research Council through the Darksurvey grant[614030] ; UK Science and Technology Facilities Council[ST/N000668/1] ; UK Space Agency[ST/N00180X/1] ; 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 ; 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 ; Pennsylvania State University ; Princeton University ; Spanish Participation Group ; Yale University ; 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-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; New Mexico State University ; Shanghai Astronomical Observatory ; Univer-sity of Utah ; SEPNet ; University of Portsmouth ; DOE Office of Science User Facility ; Office of Science of the U.S. Department of Energy[DE-AC02-05CH11231] ; New York University ; University of Florida ; University of Tokyo ; University of Utah ; United Kingdom Participation Group
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000462280000070
资助机构European Research Council through the Darksurvey grant ; European Research Council through the Darksurvey grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; 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 ; 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 ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; Yale University ; Yale University ; 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-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; New Mexico State University ; New Mexico State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; Univer-sity of Utah ; Univer-sity of Utah ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; New York University ; New York University ; University of Florida ; University of Florida ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; United Kingdom Participation Group ; United Kingdom Participation Group ; European Research Council through the Darksurvey grant ; European Research Council through the Darksurvey grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; 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 ; 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 ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; Yale University ; Yale University ; 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-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; New Mexico State University ; New Mexico State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; Univer-sity of Utah ; Univer-sity of Utah ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; New York University ; New York University ; University of Florida ; University of Florida ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; United Kingdom Participation Group ; United Kingdom Participation Group ; European Research Council through the Darksurvey grant ; European Research Council through the Darksurvey grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; 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 ; 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 ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; Yale University ; Yale University ; 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-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; New Mexico State University ; New Mexico State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; Univer-sity of Utah ; Univer-sity of Utah ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; New York University ; New York University ; University of Florida ; University of Florida ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; United Kingdom Participation Group ; United Kingdom Participation Group ; European Research Council through the Darksurvey grant ; European Research Council through the Darksurvey grant ; UK Science and Technology Facilities Council ; UK Science and Technology Facilities Council ; UK Space Agency ; UK Space Agency ; 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 ; 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 ; Pennsylvania State University ; Pennsylvania State University ; Princeton University ; Princeton University ; Spanish Participation Group ; Spanish Participation Group ; Yale University ; Yale University ; 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-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-PlanckInstitut fuer Extraterrestrische Physik (MPE) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fuer Astronomie (MPIA Heidelberg) ; New Mexico State University ; New Mexico State University ; Shanghai Astronomical Observatory ; Shanghai Astronomical Observatory ; Univer-sity of Utah ; Univer-sity of Utah ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; DOE Office of Science User Facility ; DOE Office of Science User Facility ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; New York University ; New York University ; University of Florida ; University of Florida ; University of Tokyo ; University of Tokyo ; University of Utah ; University of Utah ; United Kingdom Participation Group ; United Kingdom Participation Group
源URL[http://ir.bao.ac.cn/handle/114a11/25699]  
专题中国科学院国家天文台
通讯作者Ruggeri, Rossana
作者单位1.Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
2.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
3.Sorbonne Univ, ILP, 98 Bis Blvd Arago, F-75014 Paris, France
4.Univ Paris 06, Lab Phys Nucl & Hautes Energies, 4 Pl Jussieu, F-75005 Paris, France
5.Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
6.Yale Univ, Dept Phys, New Haven, CT 06511 USA
7.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
8.Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
9.Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85741 Garching, Germany
10.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
推荐引用方式
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Ruggeri, Rossana,Percival, Will J.,Gil-Marin, Hector,et al. The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift-space distortions between redshift 0.8 and 2.2[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2019,483(3):3878-3887.
APA Ruggeri, Rossana.,Percival, Will J..,Gil-Marin, Hector.,Beutler, Florian.,Mueller, Eva-Maria.,...&Zhao, Cheng.(2019).The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift-space distortions between redshift 0.8 and 2.2.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,483(3),3878-3887.
MLA Ruggeri, Rossana,et al."The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measuring the evolution of the growth rate using redshift-space distortions between redshift 0.8 and 2.2".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 483.3(2019):3878-3887.

入库方式: OAI收割

来源:国家天文台

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