NAOC Open IR
The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the halo occupation distribution model for emission line galaxies
Avila, S.1,2,3; Gonzalez-Perez, V3,4; Mohammad, F. G.5,6; de Mattia, A.7; Zhao, C.8; Raichoor, A.8; Tamone, A.8; Alam, S.9; Bautista, J.3; Bianchi, D.10,11; Burtin, E.7; Chapman, M. J.5,6; Chuang, C-H12; Comparat, J.13; Dawson, K.14; Divers, T.3; des Bourboux, H. du Mas14; Gil-Marin, H.10,11; Mueller, E. M.15; Habib, S.16; Heitmann, K.16; Ruhlmann-Kleider, V7; Padilla, N.17; Percival, W. J.5,6,18; Ross, A. J.19; Seo, H. J.19; Schneider, D. P.20; Zhao, G.3,21
2020-12-01
Source PublicationMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
ISSN0035-8711
Volume499Issue:4Pages:5486-5507
AbstractWe study the modelling of the halo occupation distribution (HOD) for the eBOSS DR16 emission line galaxies (ELGs). Motivated by previous theoretical and observational studies, we consider different physical effects that can change how ELGs populate haloes. We explore the shape of the average HOD, the fraction of satellite galaxies, their probability distribution function (PDF), and their density and velocity profiles, Our baseline HOD shape was fitted to a semi-analytical model of galaxy formation and evolution, with a decaying occupation of central ELGs at high halo masses. We consider Poisson and sub/super-Poissonian PDFs for satellite assignment. We model both Navarro-Frenk-White and particle profiles for satellite positions, also allowing for decreased concentrations, We model velocities with the virial theorem and particle velocity distributions. Additionally, we introduce a velocity bias and a net in fall velocity. We study how these choices impact the clustering statistics while keeping the number density and bias fixed to that from eBOSS ELGs, The projected correlation function, w(p), captures most of the effects from the PDF and satellites profile. The quadrupole, xi(2), captures most of the effects coming from the velocity profile. We find that the impact of the mean HOD shape is subdominant relative to the rest of choices, We fit the clustering of the eBOSS DR16 ELG data under different combinations of the above assumptions. The catalogues presented here have been analysed in companion papers, showing that eBOSS RSD+BAO measurements are insensitive to the details of galaxy physics considered here. These catalogues are made publicly available.
Keywordmethods: analytical methods: numerical galaxies: evolution galaxies: haloes cosmology: theory large-scale structure of the Universe
Funding OrganizationMICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University
DOI10.1093/mnras/staa2951
WOS KeywordLARGE-SCALE STRUCTURE ; GALACTIC CONFORMITY ; POWER-SPECTRUM ; ASSEMBLY BIAS ; EVOLUTION ; CATALOGS ; LUMINOSITY ; DEPENDENCE ; FILAMENTS ; EMITTERS
Language英语
Funding ProjectMICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions[713366] ; European Research Council (ERC) under European Union[769130] ; European Research Council through the COSFORM Research Grant[670193] ; ERC under European Union[693024] ; Alfred P. Sloan Foundation ; U.S. Department of Energy Office of Science ; Center for High-Performance Computing at the University of Utah ; Brazilian Participation Group ; Carnegie Institution for Science ; Chilean Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; New Mexico State University ; New York University ; University of Notre Dame ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Colorado Boulder ; University of Oxford ; University of Portsmouth ; University of Utah ; University ofVirginia ; University ofWashington ; University of Wisconsin ; Vanderbilt University ; Yale University ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy[DE-AC02-05CH11231] ; Carnegie Mellon University
Funding OrganizationMICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; MICUES project - European Union's Horizon 2020 research programme under the H2020 Marie Sklodowska-Curie Actions ; European Research Council (ERC) under European Union ; European Research Council (ERC) under European Union ; European Research Council through the COSFORM Research Grant ; European Research Council through the COSFORM Research Grant ; ERC under European Union ; ERC under European Union ; 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 ; Brazilian Participation Group ; Brazilian Participation Group ; Carnegie Institution for Science ; Carnegie Institution for Science ; Chilean Participation Group ; Chilean Participation Group ; French Participation Group ; French Participation Group ; Harvard-Smithsonian Center for Astrophysics ; Harvard-Smithsonian Center for Astrophysics ; Instituto de Astrofisica de Canarias ; Instituto de Astrofisica de Canarias ; Johns Hopkins University ; Johns Hopkins University ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; Kavli Institute for the Physics and Mathematics of the Universe (IPMU) ; University of Tokyo ; University of Tokyo ; Korean Participation Group ; Korean Participation Group ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Leibniz Institut f ur Astrophysik Potsdam (AIP) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-Planck-Institut fur Astronomie (MPIA Heidelberg) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-PlanckInstitut fur Astrophysik (MPA Garching) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; Max-Planck-Institut f ur Extraterrestrische Physik (MPE) ; National Astronomical Observatories of China ; National Astronomical Observatories of China ; New Mexico State University ; New Mexico State University ; New York University ; New York University ; University of Notre Dame ; University of Notre Dame ; Observat ario Nacional/MCTI ; Observat ario Nacional/MCTI ; Ohio StateUniversity ; Ohio StateUniversity ; Pennsylvania State University ; Pennsylvania State University ; ShanghaiAstronomical Observatory ; ShanghaiAstronomical Observatory ; United Kingdom Participation Group ; United Kingdom Participation Group ; Universidad Nacional Aut onoma deMexico ; Universidad Nacional Aut onoma deMexico ; University of Arizona ; University of Arizona ; University of Colorado Boulder ; University of Colorado Boulder ; University of Oxford ; University of Oxford ; University of Portsmouth ; University of Portsmouth ; University of Utah ; University of Utah ; University ofVirginia ; University ofVirginia ; University ofWashington ; University ofWashington ; University of Wisconsin ; University of Wisconsin ; Vanderbilt University ; Vanderbilt University ; Yale University ; Yale University ; Institute of Cosmology and Gravitation ; Institute of Cosmology and Gravitation ; Office of Science of the U.S. Department of Energy ; Office of Science of the U.S. Department of Energy ; Carnegie Mellon University ; Carnegie Mellon University
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000599131700060
PublisherOXFORD UNIV PRESS
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/80303
Collection中国科学院国家天文台
Corresponding AuthorAvila, S.; Gonzalez-Perez, V
Affiliation1.Univ Autonoma Madrid, Fac Ciencias, Dept Fis Teor, Cantoblanco, E-28049 Madrid, Spain
2.Univ Autonoma Madrid, Inst Fis Teor, UAM, CSIC, Cantoblanco, E-28049 Madrid, Spain
3.Univ Portsmouth, Inst Cosmol & Gravitat, Dennis Sciama Bldg, Portsmouth PO1 3FX, Hants, England
4.Liverpool John Moores Univ, Astrophys Res Inst, 146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England
5.Univ Waterloo, Waterloo Ctr Astrophys, 200 Univ Ave W, Waterloo, ON N2L 3G1, Canada
6.Univ Waterloo, Dept Phys & Astron, 200 Univ Ave W, Waterloo, ON N2L 3G1, Canada
7.Univ Paris Saclay, CEA, IRFU, F-91191 Gif Sur Yvette, France
8.Ecole Polytech Fed Lausanne EPFL, Lab Astrophys, Inst Phys, CH-1290 Versoix, Switzerland
9.Univ Edinburgh, Inst Astron, Royal Observ, Edinburgh EH9 3HJ, Midlothian, Scotland
10.Univ Barcelona, IEEC UB, ICC, Marti i Branques 1, E-08028 Barcelona, Spain
11.Inst Estudis Espacials Catalunya IEEC, E-08034 Barcelona, Spain
12.Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA
13.Max Planck Inst Extraterr Phys, Postfach 1312, D-85741 Garching, Germany
14.Univ Utah, Dept Phys & Astron, 115 S 1400 E, Salt Lake City, UT 84112 USA
15.Univ Oxford, Subdept Astrophys, Dept Phys, Oxford OX1 3RH, England
16.Argonne Natl Lab, HEP Div, Lemont, IL 60439 USA
17.Pontificia Univ Catolica Chiless, Inst Astrofis, Vicuna Mackenna 4860, Santiago, Chile
18.Perimeter Inst Theoret Phys, 31 Caroline St North, Waterloo, ON N2L 2Y5, Canada
19.Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Columbus, OH 43212 USA
20.Penn State Univ, University Pk, PA 16802 USA
21.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Avila, S.,Gonzalez-Perez, V,Mohammad, F. G.,et al. The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the halo occupation distribution model for emission line galaxies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,499(4):5486-5507.
APA Avila, S..,Gonzalez-Perez, V.,Mohammad, F. G..,de Mattia, A..,Zhao, C..,...&Zhao, G..(2020).The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the halo occupation distribution model for emission line galaxies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,499(4),5486-5507.
MLA Avila, S.,et al."The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: exploring the halo occupation distribution model for emission line galaxies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 499.4(2020):5486-5507.
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