The Mass–Metallicity Relation at z?～?0.8: Redshift Evolution and Parameter Dependency

doi:10.3847/1538-4357/ab4902

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	The Mass–Metallicity Relation at z?～?0.8: Redshift Evolution and Parameter Dependency
	Huang,Chi 1,2; Zou,Hu 3; Kong,Xu 1,2; Comparat,Johan 4; Lin,Zesen 1,2; Gao,Yulong 1,2; Liang,Zhixiong 1,2; Delubac,Timothee 5; Raichoor,Anand 5; Kneib,Jean-Paul 5
刊名	The Astrophysical Journal
	2019-11-15
卷号	886 期号:1
关键词	Emission line galaxies Scaling relations Galaxy abundances
ISSN号	0004-637X
DOI	10.3847/1538-4357/ab4902
英文摘要	Abstract 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?
语种	英语
出版者	The American Astronomical Society
WOS记录号	IOP:0004-637X-886-1-ab4902
内容类型	期刊论文
源URL	[http://ir.bao.ac.cn/handle/114a11/28622]
专题	中国科学院国家天文台
作者单位	1.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
推荐引用方式 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).