Variation of the Mid-infrared versus Ha Luminosity Correlation with Increasing Redshift for Galaxies in the Local Universe
文献类型：期刊论文
| 作者 | Zhu, Yinan1,2; Wu, Hong1; Jin, Junjie1,3 |
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2019-03-20 |
| 卷号 | 874期号:1页码:14 |
| 关键词 | galaxies: starburst infrared: galaxies stars: formation |
| ISSN号 | 0004-637X |
| DOI | 10.3847/1538-4357/ab04a1 |
| 英文摘要 | The correlation between mid-infrared (MIR) and Ha luminosity (hereafter referred to as the MIR versus Ha correlation) has been investigated for years, and these approximate linear correlations have been applied to many studies to derive the ongoing star formation rate (SFR) for galaxies near and far. We present and analyze the correlations between rest-frame 12 and 22 mu m and Ha luminosities for a large sample of star-forming galaxies with redshift ranging from 0.03 to 0.15 selected in the cross-matched SDSS DR7 and ALLWISE survey. For the galaxies located in a relatively narrow redshift bin (Delta z similar to 0.01), we find that the fitting slope of the MIR versus Ha correlation is always less than 1, and less than the slope derived for all the star-forming galaxies covering a broad redshift range (0.03 < z < 0.15). Additionally, the fitting intercept increases with redshift. We check the influence on the L[MIR] versus L[H alpha] correlation from K- and aperture correction, the variation of either star formation history or morphology, and find their influence is not large enough to account for the inconsistency of the MIR versus Ha correlation individually. We also find that there is possible evolution for the SFR versus M* (stellar mass) correlation within the redshift coverage from 0.03 to 0.15. Finally, we warn that an unwanted error might be brought in if the MIR versus Ha correlation derived from the sample covering a large redshift interval has been applied, and indicate an explicit study is needed to establish an accurate, redshift-independent MIR versus Ha correlation. |
| WOS关键词 | STAR-FORMATION RATES ; DIGITAL SKY SURVEY ; DUST EMISSION ; HOST GALAXIES ; NGC-5194 M51A ; STELLAR MASS ; IR EMISSION ; SPITZER ; CLASSIFICATION ; SPECTRA |
| 资助项目 | National Key R&D Program of China[2017YFA0402704] ; NSFC[11733006] ; Alfred P. Sloan Foundation ; National Science Foundation ; U.S. Department of Energy ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Max Planck Society ; Higher Education Funding Council for England ; American Museum of Natural History ; Astrophysical Institute Potsdam ; University of Basel ; University of Cambridge ; Case Western Reserve University ; University of Chicago ; Drexel University ; Fermilab ; Institute for Advanced Study ; Japan Participation Group, Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; Ohio State University ; University of Pittsburgh ; University of Portsmouth ; Princeton University ; United States Naval Observatory ; University of Washington |
| WOS研究方向 | Astronomy & Astrophysics |
| 语种 | 英语 |
| WOS记录号 | WOS:000462602500012 |
| 出版者 | IOP PUBLISHING LTD |
| 资助机构 | National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; Case Western Reserve University ; Case Western Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group, Johns Hopkins University ; Japan Participation Group, Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; Case Western Reserve University ; Case Western Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group, Johns Hopkins University ; Japan Participation Group, Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; Case Western Reserve University ; Case Western Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group, Johns Hopkins University ; Japan Participation Group, Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington ; National Key R&D Program of China ; National Key R&D Program of China ; NSFC ; NSFC ; Alfred P. Sloan Foundation ; Alfred P. Sloan Foundation ; National Science Foundation ; National Science Foundation ; U.S. Department of Energy ; U.S. Department of Energy ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; Japanese Monbukagakusho ; Japanese Monbukagakusho ; Max Planck Society ; Max Planck Society ; Higher Education Funding Council for England ; Higher Education Funding Council for England ; American Museum of Natural History ; American Museum of Natural History ; Astrophysical Institute Potsdam ; Astrophysical Institute Potsdam ; University of Basel ; University of Basel ; University of Cambridge ; University of Cambridge ; Case Western Reserve University ; Case Western Reserve University ; University of Chicago ; University of Chicago ; Drexel University ; Drexel University ; Fermilab ; Fermilab ; Institute for Advanced Study ; Institute for Advanced Study ; Japan Participation Group, Johns Hopkins University ; Japan Participation Group, Johns Hopkins University ; Joint Institute for Nuclear Astrophysics ; Joint Institute for Nuclear Astrophysics ; Kavli Institute for Particle Astrophysics and Cosmology ; Kavli Institute for Particle Astrophysics and Cosmology ; Korean Scientist Group ; Korean Scientist Group ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astronomy (MPIA) ; Max-Planck-Institute for Astrophysics (MPA) ; Max-Planck-Institute for Astrophysics (MPA) ; New Mexico State University ; New Mexico State University ; Ohio State University ; Ohio State University ; University of Pittsburgh ; University of Pittsburgh ; University of Portsmouth ; University of Portsmouth ; Princeton University ; Princeton University ; United States Naval Observatory ; United States Naval Observatory ; University of Washington ; University of Washington |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/25762]  |
| 专题 | 中国科学院国家天文台 |
| 通讯作者 | Zhu, Yinan |
| 作者单位 | 1.Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100101, Peoples R China 2.Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China 3.Univ Chinese Acad Sci, Sch Astron & Space Sci, Beijing 100039, Peoples R China |
| 推荐引用方式 GB/T 7714 | Zhu, Yinan,Wu, Hong,Jin, Junjie. Variation of the Mid-infrared versus Ha Luminosity Correlation with Increasing Redshift for Galaxies in the Local Universe[J]. ASTROPHYSICAL JOURNAL,2019,874(1):14. |
| APA | Zhu, Yinan,Wu, Hong,&Jin, Junjie.(2019).Variation of the Mid-infrared versus Ha Luminosity Correlation with Increasing Redshift for Galaxies in the Local Universe.ASTROPHYSICAL JOURNAL,874(1),14. |
| MLA | Zhu, Yinan,et al."Variation of the Mid-infrared versus Ha Luminosity Correlation with Increasing Redshift for Galaxies in the Local Universe".ASTROPHYSICAL JOURNAL 874.1(2019):14. |
入库方式： OAI收割
来源：国家天文台
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