NAOC Open IR
Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey - I: Catalogue preparation and systematic mitigation
Rezaie, Mehdi1; Ross, Ashley J.2; Seo, Hee-Jong1; Mueller, Eva-Maria3; Percival, Will J.4,5,6; Merz, Grant1; Katebi, Reza1; Bunescu, Razvan C.7; Bautista, Julian8; Brownstein, Joel R.9; Burtin, Etienne10; Dawson, Kyle9; Gil-Marin, Hector11,12; Hou, Jiamin13; Lyke, Eleanor B.14; de la Macorra, Axel15; Rossi, Graziano16; Schneider, Donald P.17,18; Zarrouk, Pauline10,19; Zhao, Gong-Bo20,21
2021-09-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume506Issue:3Pages:3439-3454
AbstractWe investigate the large-scale clustering of the final spectroscopic sample of quasars from the recently completed extended Baryon Oscillation Spectroscopic Survey (eBOSS). The sample contains 343 708 objects in the redshift range 0.8 < z < 2.2 and 72 667 objects with redshifts 2.2 < z < 3.5, covering an effective area of 4699 deg(2). We develop a neural network-based approach to mitigate spurious fluctuations in the density field caused by spatial variations in the quality of the imaging data used to select targets for follow-up spectroscopy. Simulations are used with the same angular and radial distributions as the real data to estimate covariance matrices, perform error analyses, and assess residual systematic uncertainties. We measure the mean density contrast and cross-correlations of the eBOSS quasars against maps of potential sources of imaging systematics to address algorithm effectiveness, finding that the neural network-based approach outperforms standard linear regression. Stellar density is one of the most important sources of spurious fluctuations, and a new template constructed using data from the Gaia spacecraft provides the best match to the observed quasar clustering. The end-product from this work is a new value-added quasar catalogue with the improved weights to correct for non-linear imaging systematic effects, which will be made public. Our quasar catalogue is used to measure the local-type primordial non-Gaussianity in a companion paper.
Keywordinflation large-scale structure of the Universe
Funding OrganizationU.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University
DOI10.1093/mnras/stab1730
WOS KeywordPOWER-SPECTRUM ANALYSIS ; LARGE-SCALE STRUCTURE ; LY-ALPHA ABSORPTION ; ACOUSTIC-OSCILLATIONS ; DENSITY PERTURBATIONS ; DATA RELEASE ; REDSHIFT MEASUREMENT ; FIBER COLLISIONS ; GALAXIES ; QUASARS
Language英语
Funding ProjectU.S. Department of Energy, Office of Science, Office of High Energy Physics[DE-SC0014329] ; U.S. Department of Energy, Office of Science, Office of High Energy Physics[DE-SC0019091] ; National Research Foundation of Korea (NRF)[2017R1E1A1A01077508] ; National Research Foundation of Korea (NRF)[2020R1A2C1005655] ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility[DE-AC02-05CH11231] ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University
Funding OrganizationU.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; U.S. Department of Energy, Office of Science, Office of High Energy Physics ; National Research Foundation of Korea (NRF) ; National Research Foundation of Korea (NRF) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; theKorean Ministry of Education, Science andTechnology (MoEST) ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; U.S. Department of Energy, Office of Science ; U.S. Department of Energy, Office of Science ; Center for High Performance Computing at the University of Utah ; Center for High Performance Computing at the University of Utah ; National Energy Research Scientific Computing Center (NERSC) ; National Energy Research Scientific Computing Center (NERSC) ; NERSC is a U.S. Department of Energy Office of Science User Facility ; NERSC is a U.S. Department of Energy Office of Science User Facility ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics | Harvard ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut f ur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; Max-Planck-Institut fur Extraterrestrische Physik (MPE) ; NewMexico State University, New York University ; NewMexico State University, New York University ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Aut PRIME ; Yale University ; Yale University
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000685245200025
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/75921
Collection中国科学院国家天文台
Corresponding AuthorRezaie, Mehdi
Affiliation1.Ohio Univ, Dept Phys & Astron, Athens, OH 45701 USA
2.Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43210 USA
3.Univ Oxford, Dept Phys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
4.Univ Waterloo, Waterloo Ctr Astrophys, Waterloo, ON N2L 3G1, Canada
5.Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
6.Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
7.Univ N Carolina, Coll Comp & Informat, Dept Comp Sci, Charlotte, NC 28223 USA
8.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
9.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
10.Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
11.Univ Barcelona, Inst Ciencies Cosmos, ICCUB, Marti & Franques 1, E-08028 Barcelona, Spain
12.Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain
13.Max Planck Inst Extraterr Phys, Postfach 1312,Giessenbachstr, D-85748 Garching, Germany
14.Univ Wyoming, Dept Phys & Astron, Laramie, WY 82071 USA
15.Univ Nacl Autonoma Mexico, Inst Fis, Apdo Postal 20-364, Ciudad De Mexico, Mexico
16.Sejong Univ, Dept Phys & Astron, Seoul 143747, South Korea
17.Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
18.Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
19.Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, England
20.Chinese Acad Sci, Natl Astron Observ, Beijing 100101, Peoples R China
21.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100049, Peoples R China
Recommended Citation
GB/T 7714
Rezaie, Mehdi,Ross, Ashley J.,Seo, Hee-Jong,et al. Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey - I: Catalogue preparation and systematic mitigation[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2021,506(3):3439-3454.
APA Rezaie, Mehdi.,Ross, Ashley J..,Seo, Hee-Jong.,Mueller, Eva-Maria.,Percival, Will J..,...&Zhao, Gong-Bo.(2021).Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey - I: Catalogue preparation and systematic mitigation.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,506(3),3439-3454.
MLA Rezaie, Mehdi,et al."Primordial non-Gaussianity from the completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey - I: Catalogue preparation and systematic mitigation".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 506.3(2021):3439-3454.
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