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tokens: This work uses data obtained through the Telescope Access Program (TAP), which is funded by the National Astronomical Observatories of China, the Chinese Academy of Sciences (the Strategic Priority Research Program, “The Emergence of Cosmological Structures” Grant No. XDB09000000), and the Special Fund for Astronomy from the Ministry of Finance. The observations reported in this study were obtained at the MMT Observatory, a joint facility of the Smithsonian Institution and the University of Arizona. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work is supported by the National Basic Research Program of China (973 Program)(2015CB857004), and the National Natural Science Foundation of China (NSFC, Nos. 1320101002, 11433005, 11421303, and 11673004), and the Yunnan Applied Basic Research Projects (2014FB155). E.W. was supported by the Youth Innovation Fund by the University of Science and Technology of China (No. WK2030220019). Facility: MMT. Software: SExtractor (Bertin Arnouts 1996 ), xfitfibs, HSRED, STARLIGHT (Cid Fernandes et al. 2005 ), MPFIT (Markwardt 2009 ), PyNeb (Luridiana et al. 2015 ).