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A large, deep 3 deg2 survey of H alpha, [O III], and [O II] emitters from LAGER: constraining luminosity functions

文献类型：期刊论文

作者Khostovan, A. A.1; Malhotra, S.1,2; Rhoads, J. E.1,2; Jiang, C.3; Wang, J.4; Wold, I.1; Zheng, Z. -Y.3; Barrientos, L. F.5; Coughlin, A.2,6; Harish, S.2
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2020-04-01
卷号493期号:3页码:3966-3984
ISSN号0035-8711
关键词galaxies: evolution galaxies: high-redshift galaxies: star formation cosmology: observations
英文摘要We present our measurements of the Ha, [01111, and [OW luminosity functions as part of the Lyman Alpha Galaxies at Epoch of Reionization (LAGER) survey using our samples of 1577 z = 0.47 H a-, 3933 z = 0.93 [0 and 5367 z = 1,59 [0 u1 -selected emission line galaxies in a 3 deg2 single, CHO/Blanco DECam pointing of the COSMOS field, Our observations reach 50- depths of 8.2 x 10-18 erg s -I cm -2 and comoving volumes of (1-7) x 105 Mpc3 making our survey one of the deepest narrow -hand surveys. We select our emission line galaxies via spectroscopic confirmation, photometric redshifts, and colour-colour selections. We measure 316_'_;.`99the observed luminosity functions for each sample and find best fits of (p* = 10-- Mpc-3 and L* = 1041.72"a erg s -I for Ha, (/)* = 1 0-2.161i M c'1 and L* = 1041.38Z6 erg s-1 for [0111], and (/5* = 10 1.971,.i1041.66 'Mpc-3 and L* = erg s -I for [Oil], with a fixed to - 1.75, -1.6, and -1,3, respectively. An excess of bright >1042 erg s -I [0111] emitters is observed and may be due to active galactic nucleus (AGN) contamination, Corrections for dust attenuation are applied assuming Afp, = 1 mag. We also design our own empirical rest frame g - r calibration using SDSS DR12 data, test it against our z = 0,47 H a emitters with zCOSMOS 1D spectra, and calibrate it for (g - r) between -0.8 and 1.3 mag. Dust and AGNcorrected star formation rate densities (SERDs) are measured as logiopsFRAM(.; yr I Mpc-3) = - 1,63 + 0,04, -1.07 + 0,06, and -0.90 + 0.10 for H a, [0 in and [Ou], respectively. We find our [0 uf] and [0 RI samples fully trace cosmic star formation activity at their respective redshifts in comparison to multiwavelength SERDs, while the Ha sample traces =70 per cent of the total z = 0,47 SURD,
WOS关键词STAR-FORMATION RATE ; WIDE-FIELD SURVEY ; HIGH-REDSHIFT SURVEY ; SIMILAR-TO 5 ; FORMING GALAXIES ; COSMOS FIELD ; STELLAR MASS ; HOMOGENEOUS MEASURE ; GOODS FIELD ; X-RAY
资助项目US National Science Foundation[AST-1518057] ; NASA via WFIRST Preparatory Science Grant[NNX15AJ79G] ; NASA via WFIRST Science Investigation Team[NNG16PJ33C] ; CONICYT[BASAL AFB-17000] ; CAS Key Research Program of Frontier Sciences[QYZDB-SSW-SYS033] ; NSFC[11421303] ; NSFC[11890693] ; Shanghai Pujiang Program ; National Science Foundation of China[11773051] ; CAS Pioneer Hundred Talents Program ; U.S. Department of Energy ; U.S. National Science Foundation ; Ministry of Science and Education of Spain ; Science and Technology Facilities Council of the United Kingdom ; Higher Education Funding Council for England ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; Kavli Institute of Cosmological Physics at the University of Chicago ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Financiadora de Estudos e Projetos ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Ministerio da Ciencia, Tecnologia e Inovacao ; Deutsche Forschungsgemeinschaft ; Argonne National Laboratory ; University of California at Santa Cruz ; University of Cambridge ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; University of Chicago ; University College London ; DES-Brazil Consortium ; University of Edinburgh ; Eidgenossische Technische Hochschule (ETH) Zurich ; Fermi National Accelerator Laboratory ; University of Illinois at Urbana-Champaign ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Fisica d'Altes Energies ; Lawrence Berkeley National Laboratory ; Ludwig-Maximilians Universitat Munchen ; associated Excellence Cluster Universe ; University of Michigan ; National Optical Astronomy Observatory ; University of Nottingham ; Ohio State University ; OzDES Membership Consortium ; University of Pennsylvania ; University of Portsmouth ; SLAC National Accelerator Laboratory ; Stanford University ; University of Sussex ; Texas AM University
WOS研究方向Astronomy & Astrophysics
语种英语
出版者OXFORD UNIV PRESS
WOS记录号WOS:000526035600064
资助机构US National Science Foundation ; US National Science Foundation ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Science Investigation Team ; NASA via WFIRST Science Investigation Team ; CONICYT ; CONICYT ; CAS Key Research Program of Frontier Sciences ; CAS Key Research Program of Frontier Sciences ; NSFC ; NSFC ; Shanghai Pujiang Program ; Shanghai Pujiang Program ; National Science Foundation of China ; National Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. National Science Foundation ; U.S. National Science Foundation ; Ministry of Science and Education of Spain ; Ministry of Science and Education of Spain ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; Kavli Institute of Cosmological Physics at the University of Chicago ; Kavli Institute of Cosmological Physics at the University of Chicago ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Financiadora de Estudos e Projetos ; Financiadora de Estudos e Projetos ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Ministerio da Ciencia, Tecnologia e Inovacao ; Ministerio da Ciencia, Tecnologia e Inovacao ; Deutsche Forschungsgemeinschaft ; Deutsche Forschungsgemeinschaft ; Argonne National Laboratory ; Argonne National Laboratory ; University of California at Santa Cruz ; University of California at Santa Cruz ; University of Cambridge ; University of Cambridge ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; University of Chicago ; University of Chicago ; University College London ; University College London ; DES-Brazil Consortium ; DES-Brazil Consortium ; University of Edinburgh ; University of Edinburgh ; Eidgenossische Technische Hochschule (ETH) Zurich ; Eidgenossische Technische Hochschule (ETH) Zurich ; Fermi National Accelerator Laboratory ; Fermi National Accelerator Laboratory ; University of Illinois at Urbana-Champaign ; University of Illinois at Urbana-Champaign ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Fisica d'Altes Energies ; Institut de Fisica d'Altes Energies ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Ludwig-Maximilians Universitat Munchen ; Ludwig-Maximilians Universitat Munchen ; associated Excellence Cluster Universe ; associated Excellence Cluster Universe ; University of Michigan ; University of Michigan ; National Optical Astronomy Observatory ; National Optical Astronomy Observatory ; University of Nottingham ; University of Nottingham ; Ohio State University ; Ohio State University ; OzDES Membership Consortium ; OzDES Membership Consortium ; University of Pennsylvania ; University of Pennsylvania ; University of Portsmouth ; University of Portsmouth ; SLAC National Accelerator Laboratory ; SLAC National Accelerator Laboratory ; Stanford University ; Stanford University ; University of Sussex ; University of Sussex ; Texas AM University ; Texas AM University ; US National Science Foundation ; US National Science Foundation ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Science Investigation Team ; NASA via WFIRST Science Investigation Team ; CONICYT ; CONICYT ; CAS Key Research Program of Frontier Sciences ; CAS Key Research Program of Frontier Sciences ; NSFC ; NSFC ; Shanghai Pujiang Program ; Shanghai Pujiang Program ; National Science Foundation of China ; National Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. National Science Foundation ; U.S. National Science Foundation ; Ministry of Science and Education of Spain ; Ministry of Science and Education of Spain ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; Kavli Institute of Cosmological Physics at the University of Chicago ; Kavli Institute of Cosmological Physics at the University of Chicago ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Financiadora de Estudos e Projetos ; Financiadora de Estudos e Projetos ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Ministerio da Ciencia, Tecnologia e Inovacao ; Ministerio da Ciencia, Tecnologia e Inovacao ; Deutsche Forschungsgemeinschaft ; Deutsche Forschungsgemeinschaft ; Argonne National Laboratory ; Argonne National Laboratory ; University of California at Santa Cruz ; University of California at Santa Cruz ; University of Cambridge ; University of Cambridge ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; University of Chicago ; University of Chicago ; University College London ; University College London ; DES-Brazil Consortium ; DES-Brazil Consortium ; University of Edinburgh ; University of Edinburgh ; Eidgenossische Technische Hochschule (ETH) Zurich ; Eidgenossische Technische Hochschule (ETH) Zurich ; Fermi National Accelerator Laboratory ; Fermi National Accelerator Laboratory ; University of Illinois at Urbana-Champaign ; University of Illinois at Urbana-Champaign ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Fisica d'Altes Energies ; Institut de Fisica d'Altes Energies ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Ludwig-Maximilians Universitat Munchen ; Ludwig-Maximilians Universitat Munchen ; associated Excellence Cluster Universe ; associated Excellence Cluster Universe ; University of Michigan ; University of Michigan ; National Optical Astronomy Observatory ; National Optical Astronomy Observatory ; University of Nottingham ; University of Nottingham ; Ohio State University ; Ohio State University ; OzDES Membership Consortium ; OzDES Membership Consortium ; University of Pennsylvania ; University of Pennsylvania ; University of Portsmouth ; University of Portsmouth ; SLAC National Accelerator Laboratory ; SLAC National Accelerator Laboratory ; Stanford University ; Stanford University ; University of Sussex ; University of Sussex ; Texas AM University ; Texas AM University ; US National Science Foundation ; US National Science Foundation ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Science Investigation Team ; NASA via WFIRST Science Investigation Team ; CONICYT ; CONICYT ; CAS Key Research Program of Frontier Sciences ; CAS Key Research Program of Frontier Sciences ; NSFC ; NSFC ; Shanghai Pujiang Program ; Shanghai Pujiang Program ; National Science Foundation of China ; National Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. National Science Foundation ; U.S. National Science Foundation ; Ministry of Science and Education of Spain ; Ministry of Science and Education of Spain ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; Kavli Institute of Cosmological Physics at the University of Chicago ; Kavli Institute of Cosmological Physics at the University of Chicago ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Financiadora de Estudos e Projetos ; Financiadora de Estudos e Projetos ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Ministerio da Ciencia, Tecnologia e Inovacao ; Ministerio da Ciencia, Tecnologia e Inovacao ; Deutsche Forschungsgemeinschaft ; Deutsche Forschungsgemeinschaft ; Argonne National Laboratory ; Argonne National Laboratory ; University of California at Santa Cruz ; University of California at Santa Cruz ; University of Cambridge ; University of Cambridge ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; University of Chicago ; University of Chicago ; University College London ; University College London ; DES-Brazil Consortium ; DES-Brazil Consortium ; University of Edinburgh ; University of Edinburgh ; Eidgenossische Technische Hochschule (ETH) Zurich ; Eidgenossische Technische Hochschule (ETH) Zurich ; Fermi National Accelerator Laboratory ; Fermi National Accelerator Laboratory ; University of Illinois at Urbana-Champaign ; University of Illinois at Urbana-Champaign ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Fisica d'Altes Energies ; Institut de Fisica d'Altes Energies ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Ludwig-Maximilians Universitat Munchen ; Ludwig-Maximilians Universitat Munchen ; associated Excellence Cluster Universe ; associated Excellence Cluster Universe ; University of Michigan ; University of Michigan ; National Optical Astronomy Observatory ; National Optical Astronomy Observatory ; University of Nottingham ; University of Nottingham ; Ohio State University ; Ohio State University ; OzDES Membership Consortium ; OzDES Membership Consortium ; University of Pennsylvania ; University of Pennsylvania ; University of Portsmouth ; University of Portsmouth ; SLAC National Accelerator Laboratory ; SLAC National Accelerator Laboratory ; Stanford University ; Stanford University ; University of Sussex ; University of Sussex ; Texas AM University ; Texas AM University ; US National Science Foundation ; US National Science Foundation ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Preparatory Science Grant ; NASA via WFIRST Science Investigation Team ; NASA via WFIRST Science Investigation Team ; CONICYT ; CONICYT ; CAS Key Research Program of Frontier Sciences ; CAS Key Research Program of Frontier Sciences ; NSFC ; NSFC ; Shanghai Pujiang Program ; Shanghai Pujiang Program ; National Science Foundation of China ; National Science Foundation of China ; CAS Pioneer Hundred Talents Program ; CAS Pioneer Hundred Talents Program ; U.S. Department of Energy ; U.S. Department of Energy ; U.S. National Science Foundation ; U.S. National Science Foundation ; Ministry of Science and Education of Spain ; Ministry of Science and Education of Spain ; Science and Technology Facilities Council of the United Kingdom ; Science and Technology Facilities Council of the United Kingdom ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; National Center for SupercomputingApplications at theUniversity of Illinois at Urbana-Champaign ; Kavli Institute of Cosmological Physics at the University of Chicago ; Kavli Institute of Cosmological Physics at the University of Chicago ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Center for Cosmology and Astro-Particle Physics at the Ohio State University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University ; Financiadora de Estudos e Projetos ; Financiadora de Estudos e Projetos ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Fundacao Carlos Chagas Filho de Amparo a Pesquisa do Estado do Rio de Janeiro ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Conselho Nacional de Desenvolvimento Cientifico e Tecnologico ; Ministerio da Ciencia, Tecnologia e Inovacao ; Ministerio da Ciencia, Tecnologia e Inovacao ; Deutsche Forschungsgemeinschaft ; Deutsche Forschungsgemeinschaft ; Argonne National Laboratory ; Argonne National Laboratory ; University of California at Santa Cruz ; University of California at Santa Cruz ; University of Cambridge ; University of Cambridge ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas-Madrid ; University of Chicago ; University of Chicago ; University College London ; University College London ; DES-Brazil Consortium ; DES-Brazil Consortium ; University of Edinburgh ; University of Edinburgh ; Eidgenossische Technische Hochschule (ETH) Zurich ; Eidgenossische Technische Hochschule (ETH) Zurich ; Fermi National Accelerator Laboratory ; Fermi National Accelerator Laboratory ; University of Illinois at Urbana-Champaign ; University of Illinois at Urbana-Champaign ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Ciencies de l'Espai (IEEC/CSIC) ; Institut de Fisica d'Altes Energies ; Institut de Fisica d'Altes Energies ; Lawrence Berkeley National Laboratory ; Lawrence Berkeley National Laboratory ; Ludwig-Maximilians Universitat Munchen ; Ludwig-Maximilians Universitat Munchen ; associated Excellence Cluster Universe ; associated Excellence Cluster Universe ; University of Michigan ; University of Michigan ; National Optical Astronomy Observatory ; National Optical Astronomy Observatory ; University of Nottingham ; University of Nottingham ; Ohio State University ; Ohio State University ; OzDES Membership Consortium ; OzDES Membership Consortium ; University of Pennsylvania ; University of Pennsylvania ; University of Portsmouth ; University of Portsmouth ; SLAC National Accelerator Laboratory ; SLAC National Accelerator Laboratory ; Stanford University ; Stanford University ; University of Sussex ; University of Sussex ; Texas AM University ; Texas AM University
源URL[http://ir.bao.ac.cn/handle/114a11/55743]  
专题中国科学院国家天文台
通讯作者Khostovan, A. A.
作者单位1.NASA, Astrophys Div, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
2.Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA
3.Shanghai Astron Observ, CAS Key Lab Res Galaxies & Cosmol, Shanghai 200030, Peoples R China
4.Univ Sci & Technol China, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
5.Pontificia Univ Catolica Chile, Inst Astrofis, Fac Fis, Santiago 8970117, Chile
6.Chandler Gilbert Community Coll, 2626 East Pecos Rd, Chandler, AZ 85225 USA
7.Observ Carnegie Inst Washington, Las Campanas Observ, La Serena, Chile
8.Univ Diego Portales, Nucleo Astron, Santiago, Chile
9.Natl Opt Astron Observ, 950 N Cherry Ave, Tucson, AZ 85719 USA
10.Natl Opt Astron Observ, Cerro Tololo Interamer Observ, Casilla 603, La Serena, Chile
推荐引用方式
GB/T 7714		 Khostovan, A. A.,Malhotra, S.,Rhoads, J. E.,et al. A large, deep 3 deg2 survey of H alpha, [O III], and [O II] emitters from LAGER: constraining luminosity functions[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2020,493(3):3966-3984.
APA Khostovan, A. A..,Malhotra, S..,Rhoads, J. E..,Jiang, C..,Wang, J..,...&Yang, H..(2020).A large, deep 3 deg2 survey of H alpha, [O III], and [O II] emitters from LAGER: constraining luminosity functions.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,493(3),3966-3984.
MLA Khostovan, A. A.,et al."A large, deep 3 deg2 survey of H alpha, [O III], and [O II] emitters from LAGER: constraining luminosity functions".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 493.3(2020):3966-3984.

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