NAOC Open IR
The Mass-Metallicity Relation at z similar to 1-2 and Its Dependence on the Star Formation Rate
Henry, Alaina1,2; Rafelski, Marc1,2; Ben Sunnquist1; Pirzkal, Norbert1; Pacifici, Camilla1; Atek, Hakim3; Bagley, Micaela4; Baronchelli, Ivano5; Barro, Guillermo6; Bunker, Andrew J.7,8; Colbert, James9; Dai, Y. Sophia10; Elmegreen, Bruce G.11; Elmegreen, Debra Meloy12; Finkelstein, Steven4; Kocevski, Dale13; Koekemoer, Anton1; Malkan, Matthew14; Martin, Crystal L.15; Mehta, Vihang16; Pahl, Anthony14; Papovich, Casey17; Rutkowski, Michael18; Sanchez Almeida, Jorge19; Scarlata, Claudia16; Snyder, Gregory1; Teplitz, Harry9
2021-10-01
Source PublicationASTROPHYSICAL JOURNAL
ISSN0004-637X
Volume919Issue:2Pages:29
AbstractWe present a new measurement of the gas-phase mass-metallicity relation (MZR) and its dependence on star formation rates (SFRs) at 1.3 < z < 2.3. Our sample comprises 1056 galaxies with a mean redshift of z = 1.9, identified from the Hubble Space Telescope Wide Field Camera 3 (WFC3) grism spectroscopy in the Cosmic Assembly Near-infrared Deep Extragalactic Survey and the WFC3 Infrared Spectroscopic Parallel Survey. This sample is four times larger than previous metallicity surveys at z similar to 2 and reaches an order of magnitude lower in stellar mass (10(8) M (circle dot)). Using stacked spectra, we find that the MZR evolves by 0.3 dex relative to z similar to 0.1. Additionally, we identify a subset of 49 galaxies with high signal-to-noise (S/N) spectra and redshifts between 1.3 < z < 1.5, where H alpha emission is observed along with [O iii] and [O ii]. With accurate measurements of SFR in these objects, we confirm the existence of a mass-metallicity-SFR (M-Z-SFR) relation at high redshifts. These galaxies show systematic differences from the local M-Z-SFR relation, which vary depending on the adopted measurement of the local relation. However, it remains difficult to ascertain whether these differences could be due to redshift evolution, as the local M-Z-SFR relation is poorly constrained at the masses and SFRs of our sample. Lastly, we reproduced our sample selection in the IllustrisTNG hydrodynamical simulation, demonstrating that our line flux limit lowers the normalization of the simulated MZR by 0.2 dex. We show that the M-Z-SFR relation in IllustrisTNG has an SFR dependence that is too steep by a factor of around 3.
Funding OrganizationHST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute ; HST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute ; HST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute ; HST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute
DOI10.3847/1538-4357/ac1105
WOS KeywordEXTRAGALACTIC HII-REGIONS ; GAS-PHASE METALLICITY ; STELLAR MASS ; ILLUSTRISTNG SIMULATIONS ; FORMING GALAXIES ; OXYGEN ABUNDANCE ; FUNDAMENTAL RELATION ; CHEMICAL ENRICHMENT ; FORMATION HISTORIES ; MOSDEF SURVEY
Language英语
Funding ProjectHST-AR[14580] ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program[789056] ; NSFC[10878003] ; NSFC[11933003] ; National Key R&D Program of China[2017YFA0402703] ; China Manned Space Project[CMS-CSST2021-A05] ; Hubble Space Telescope, 3D-HST Treasury Program[GO 12177] ; Hubble Space Telescope, 3D-HST Treasury Program[12328] ; CANDELS MultiCycle Treasury Program[GO 11600] ; CANDELS MultiCycle Treasury Program[11696] ; CANDELS MultiCycle Treasury Program[12283] ; CANDELS MultiCycle Treasury Program[12568] ; CANDELS MultiCycle Treasury Program[12902] ; CANDELS MultiCycle Treasury Program[13352] ; CANDELS MultiCycle Treasury Program[13517] ; CANDELS MultiCycle Treasury Program[14178] ; CANDELS MultiCycle Treasury Program[13420] ; CANDELS MultiCycle Treasury Program[14227] ; NASA through the Space Telescope Science Institute[NAS5-26555]
Funding OrganizationHST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute ; HST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute ; HST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute ; HST-AR ; HST-AR ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program ; NSFC ; NSFC ; National Key R&D Program of China ; National Key R&D Program of China ; China Manned Space Project ; China Manned Space Project ; Hubble Space Telescope, 3D-HST Treasury Program ; Hubble Space Telescope, 3D-HST Treasury Program ; CANDELS MultiCycle Treasury Program ; CANDELS MultiCycle Treasury Program ; NASA through the Space Telescope Science Institute ; NASA through the Space Telescope Science Institute
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000703690700001
PublisherIOP Publishing Ltd
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/75142
Collection中国科学院国家天文台
Corresponding AuthorHenry, Alaina
Affiliation1.Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
2.Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
3.Sorbonne Univ, CNRS, Inst Astrophys Paris, UMR7095, 98bis Blvd Arago, F-75014 Paris, France
4.Univ Texas Austin, Dept Astron, RLM 15308, Austin, TX 78712 USA
5.Univ Padua, Dipartmento Fis & Astron, Vicolo Osservatorio 1-3, I-31522 Padua, Italy
6.Univ Pacific, Dept Phys, 3601 Pacific Ave, Stockton, CA 95211 USA
7.Univ Oxford, Dept Phys, Subdept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
8.Univ Tokyo, Univ Tokyo Inst Adv Study, Kavli Inst Phys & Math Universe WPI, Kashiwa, Chiba 2778583, Japan
9.CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA
10.Chinese Acad Sci, South Amer Ctr Astron CASSACA, NAOC, 20A Datun Rd, Beijing 100101, Peoples R China
11.TJ Watson Res Ctr, IBM Res Div, 1101 Kitchawan Rd, Yorktown Hts, NY 10598 USA
12.Vassar Coll, Dept Phys & Astron, Poughkeepsie, NY 12604 USA
13.Colby Coll, Dept Phys & Astron, Waterville, ME 04901 USA
14.Univ Calif Los Angeles, Dept Phys & Astron, Los Angeles, CA 90095 USA
15.Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
16.Univ Minnesota, Minnesota Inst Astrophys, 116 Church St SE, Minneapolis, MN 55455 USA
17.Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA
18.Minnesota State Univ, Dept Phys & Astron, Mankato, MN 56001 USA
19.Inst Astrofis Canarias, E-38200 Tenerife, Spain
Recommended Citation
GB/T 7714
Henry, Alaina,Rafelski, Marc,Ben Sunnquist,et al. The Mass-Metallicity Relation at z similar to 1-2 and Its Dependence on the Star Formation Rate[J]. ASTROPHYSICAL JOURNAL,2021,919(2):29.
APA Henry, Alaina.,Rafelski, Marc.,Ben Sunnquist.,Pirzkal, Norbert.,Pacifici, Camilla.,...&Teplitz, Harry.(2021).The Mass-Metallicity Relation at z similar to 1-2 and Its Dependence on the Star Formation Rate.ASTROPHYSICAL JOURNAL,919(2),29.
MLA Henry, Alaina,et al."The Mass-Metallicity Relation at z similar to 1-2 and Its Dependence on the Star Formation Rate".ASTROPHYSICAL JOURNAL 919.2(2021):29.
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