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

Chi Huang,Hu Zou,Xu Kong,Johan Comparat,Zesen Lin,Yulong Gao,Zhixiong Liang,Timothee Delubac,Anand Raichoor,Jean-Paul Kneib,Donald P. Schneider,Xu Zhou,Qirong Yuan,Matthew A. Bershady

arxiv（2019）

引用 18|浏览72

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摘要

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;z;<;1.05 and 更多

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