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The Mass–Metallicity Relation at z?~?0.8: Redshift Evolution and Parameter Dependency
Huang,Chi1,2; Zou,Hu3; Kong,Xu1,2; Comparat,Johan4; Lin,Zesen1,2; Gao,Yulong1,2; Liang,Zhixiong1,2; Delubac,Timothee5; Raichoor,Anand5; Kneib,Jean-Paul5; Schneider,Donald P.6,7; Zhou,Xu3; Yuan,Qirong8; Bershady,Matthew A.9,10
2019-11-15
Source PublicationThe Astrophysical Journal
ISSN0004-637X
Volume886Issue:1
AbstractAbstract The spectra of emission-line galaxies from the extended Baryon Oscillation Spectroscopic Survey of the Sloan Digit Sky Survey (SDSS) are used to study the mass–metallicity relation (MZR) at z?~?0.8. The selected sample contains about 180,000 massive star-forming galaxies with 0.6?
KeywordEmission line galaxies Scaling relations Galaxy abundances
DOI10.3847/1538-4357/ab4902
Language英语
WOS IDIOP:0004-637X-886-1-ab4902
PublisherThe American Astronomical Society
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/28623
Collection中国科学院国家天文台
Affiliation1.CAS Key Laboratory for Research in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, People’s Republic of China; huangchi@mail.ustc.edu.cn
2.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, People's Republic of China; xkong@ustc.edu.cn
3.Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100012, People’s Republic of China; zouhu@nao.cas.cn
4.Max-Planck-Institut fr extraterrestrische Physik, Gieenbachstr. 1, D-85748 Garching, Germany
5.Institute of Physics, Laboratory of Astrophysics, Ecole Polytechnique Fdrale de Lausanne (EPFL), Observatoire de Sauverny, 1290 Versoix, Switzerland
6.Department of Astronomy and Astrophysics, The Pennsylvania State University, University Park, PA 16802, USA
7.Institute for Gravitation and the Cosmos, The Pennsylvania State University, University Park, PA 16802, USA
8.Department of Physics, Nanjing Normal University, WenYuan Road 1, Nanjing 210046, People's Republic of China
9.Department of Astronomy, University of Wisconsin, 475 North Charter Street, Madison, WI 53706, USA
10.South African Astronomical Observatory, Cape Town, South Africa
Recommended Citation
GB/T 7714
Huang,Chi,Zou,Hu,Kong,Xu,等. The Mass–Metallicity Relation at z?~?0.8: Redshift Evolution and Parameter Dependency[J]. The Astrophysical Journal,2019,886(1).
APA Huang,Chi.,Zou,Hu.,Kong,Xu.,Comparat,Johan.,Lin,Zesen.,...&Bershady,Matthew A..(2019).The Mass–Metallicity Relation at z?~?0.8: Redshift Evolution and Parameter Dependency.The Astrophysical Journal,886(1).
MLA Huang,Chi,et al."The Mass–Metallicity Relation at z?~?0.8: Redshift Evolution and Parameter Dependency".The Astrophysical Journal 886.1(2019).
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