NAOC Open IR
The clustering of the SDSS-IV extended baryon oscillation spectroscopic survey DR16 luminous red galaxy and emission-line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
Wang, Yuting1; Zhao, Gong-Bo1,2; Zhao, Cheng3; Philcox, Oliver H. E.4,5; Alam, Shadab6; Tamone, Amelie3; de Mattia, Arnaud7; Ross, Ashley J.8; Raichoor, Anand3; Burtin, Etienne7; Paviot, Romain9,10; de la Torre, Sylvain9; Percival, Will J.11,12,13; Dawson, Kyle S.14; Gil-Marin, Hector15,16; Bautista, Julian E.17; Hou, Jiamin18; Koyama, Kazuya17; Peacock, John A.6; Ruhlmann-Kleider, Vanina7; des Bourboux, Helion du Mas14; Chuang, Chia-Hsun19; Comparat, Johan18; Escoffier, Stephanie10; Kneib, Jean-Paul3; Mueller, Eva-Maria20; Newman, Jeffrey A.21; Rossi, Graziano22; Shafieloo, Arman23; Schneider, Donald P.24
2020-11-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume498Issue:3Pages:3470-3483
AbstractWe perform a multitracer analysis using the complete Sloan Digital Sky Survey IV (SDSS-IV) extended Baryon Oscillation Spectroscopic Survey (eBOSS) DR16 luminous red galaxy (LRG) and the DR16 emission-line galaxy (ELG) samples in the configuration space, and successfully detect a cross-correlation between the two samples, and find the growth rate to be f sigma(8)=0.342 +/- 0.085 (similar to 25 per cent accuracy) from the cross-sample alone. We perform a joint measurement of the baryonic acoustic oscillation (BAO) and redshift space distortion (RSD) parameters at a single effective redshift of z(eff) = 0.77, using the autocorrelation and cross-correlation functions of the LRG and ELG samples, and find that the comoving angular diameter distance D-M(z(eff))/r(d) = 18.85 +/- 0.38, the Hubble distance D-H(z(eff))/r(d) = 19.64 +/- 0.57, and f sigma(8)(z(eff)) = 0.432 +/- 0.038, which is consistent with a Lambda CDM model at 68 per cent CL. Compared to the single-tracer analysis on the LRG sample, the Figure of Merit of alpha(perpendicular to), alpha(parallel to), and f sigma(8) is improved by a factor of 1.11 in our multitracer analysis, and in particular, the statistical uncertainty of f sigma(8) is reduced by 11.6 percent.
Keywordcosmological parameters large scale structure of the Universe
Funding OrganizationNational Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy
DOI10.1093/mnras/staa2593
WOS KeywordPOWER-SPECTRUM ANALYSIS ; WIGGLEZ OVERLAP REGION ; COVARIANCE MATRICES ; REDSHIFT SURVEY ; ACOUSTIC-OSCILLATIONS ; HALO CONCENTRATIONS ; EXPANSION RATE ; SCALE ; DENSITY ; DEPENDENCE
Language英语
Funding ProjectNational Key Basic Research and Development Program of China[2018YFA0404503] ; NSFC[11890691] ; NSFC[11925303] ; NSFC[11720101004] ; NSFC[11673025] ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; European Research Council[670193] ; WFIRST program[NNG26PJ30C] ; WFIRST program[NNN12AA01C] ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)[2017R1E1A1A01077508] ; National Research Foundation of Korea (NRF) - Korean Ministry of Education, Science and Technology (MoEST)[2020R1A2C1005655] ; Sejong University ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; ICG ; SEPNet ; University of Portsmouth ; Office of Science of the U.S. Department of Energy[DE-AC02-05CH11231]
Funding OrganizationNational Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; National Key Basic Research and Development Program of China ; National Key Basic Research and Development Program of China ; NSFC ; NSFC ; Nebula Talents Program of NAOC ; Nebula Talents Program of NAOC ; CAS Interdisciplinary Innovation Team ; CAS Interdisciplinary Innovation Team ; European Research Council ; European Research Council ; WFIRST program ; WFIRST program ; 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) ; Sejong University ; Sejong University ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; US Department of Energy Office of Science ; US Department of Energy Office of Science ; Center for HighPerformance Computing at the University of Utah ; Center for HighPerformance Computing at the University of Utah ; ICG ; ICG ; SEPNet ; SEPNet ; University of Portsmouth ; University of Portsmouth ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000587752500030
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/80869
Collection中国科学院国家天文台
Corresponding AuthorWang, Yuting; Zhao, Gong-Bo
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
2.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
3.Ecole Polytech Fed Lausanne EPFL, Lab Astrophys, Observ Sauverny, Inst Phys, CH-1290 Versoix, Switzerland
4.Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
5.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
6.Univ Edinburgh, Royal Observ, Inst Astron, Edinburgh EH9 3HJ, Midlothian, Scotland
7.Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
8.Ohio State Univ, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA
9.Aix Marseille Univ, CNRS, LAM Lab Astrophys Marseille, 38 Rue F Joliot Curie, F-13388 Marseille 13, France
10.Aix Marseille Univ, CPPM, CNRS IN2P3, CPPM UMR 7346, F-13288 Marseille, France
11.Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada
12.Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
13.Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
14.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
15.Univ Barcelona, Inst Ciencies Cosmos, ICCUB, Marti i Franques 1, E-08028 Barcelona, Spain
16.Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain
17.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
18.Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr 1, D-85748 Garching, Germany
19.Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA
20.Univ Oxford, Dept Phys, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
21.Univ Pittsburgh, Dept Phys & Astron, PITT PACC, Pittsburgh, PA 15260 USA
22.Sejong Univ, Dept Phys & Astron, Seoul 143747, South Korea
23.Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 305348, South Korea
24.Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
Recommended Citation
GB/T 7714
Wang, Yuting,Zhao, Gong-Bo,Zhao, Cheng,et al. The clustering of the SDSS-IV extended baryon oscillation spectroscopic survey DR16 luminous red galaxy and emission-line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,498(3):3470-3483.
APA Wang, Yuting.,Zhao, Gong-Bo.,Zhao, Cheng.,Philcox, Oliver H. E..,Alam, Shadab.,...&Schneider, Donald P..(2020).The clustering of the SDSS-IV extended baryon oscillation spectroscopic survey DR16 luminous red galaxy and emission-line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,498(3),3470-3483.
MLA Wang, Yuting,et al."The clustering of the SDSS-IV extended baryon oscillation spectroscopic survey DR16 luminous red galaxy and emission-line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 498.3(2020):3470-3483.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[Wang, Yuting]'s Articles
[Zhao, Gong-Bo]'s Articles
[Zhao, Cheng]'s Articles
Baidu academic
Similar articles in Baidu academic
[Wang, Yuting]'s Articles
[Zhao, Gong-Bo]'s Articles
[Zhao, Cheng]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[Wang, Yuting]'s Articles
[Zhao, Gong-Bo]'s Articles
[Zhao, Cheng]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.