Journal
ASTROPHYSICAL JOURNAL
Volume 886, Issue 1, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.3847/1538-4357/ab4902
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Funding
- National Basic Research Program of China (973 Program) [2015CB857004, 2017YFA0402600, 2014CB845704]
- National Natural Science Foundation of China (NSFC) [11433005, 11673027, 11733007, 11320101002, 11421303, 11973038, 11873032]
- External Cooperation Program of Chinese Academy of Sciences [114A11KYSB20160057]
- National Aeronautics and Space Administration
- Alfred P. Sloan Foundation
- U.S. Department of Energy Office of Science
- Center for High-Performance Computing at the University of Utah
- Brazilian Participation Group
- Carnegie Institution for Science
- Carnegie Mellon University
- Chilean Participation Group
- French Participation Group
- Harvard-Smithsonian Center for Astrophysics
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
- Korean Participation Group
- Lawrence Berkeley National Laboratory
- Leibniz Institut fur Astrophysik Potsdam (AIP)
- Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
- Max-Planck-Institut fur Astrophysik (MPA Garching)
- Max-Planck-Institut fur Extraterrestrische Physik (MPE)
- National Astronomical Observatories of China
- New Mexico State University
- New York University
- University of Notre Dame
- Observatorio Nacional/MCTI
- Ohio State University
- Pennsylvania State University
- Shanghai Astronomical Observatory
- United Kingdom Participation Group
- Universidad Nacional Autonoma de Mexico
- University of Arizona
- University of Colorado Boulder
- University of Oxford
- University of Portsmouth
- University of Utah
- University of Virginia
- University of Washington
- University of Wisconsin
- Vanderbilt University
- Yale University
- Dark Energy Camera Legacy Survey (DECaLS) [2014B-0404]
- Beijing-Arizona Sky Survey (BASS) [2015A-0801]
- Mayall z-band Legacy Survey (MzLS) [2016A-0453]
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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
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