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tokens: This work is supported by the SOC program (CHINARE2012-02-03), the NSFC grant (NSF11033007), National Basic Research Program of China (973 Program, 2013CB834905, 2015CB857005), and Fundamental Research Funds for the Central Universities (WK 2030220010). P.J. acknowledges support from the National Science Foundation of China with Grants NSFC 11233002 and NSFC11203022, the Fundamental Research Funds for the Central Universities, and the China Postdoctoral Science Foundation. Data from NED, NIST, and SDSS were used. This research uses data obtained through the Telescope Access Program (TAP), which has been funded by the Strategic Priority Research Program “The Emergence of Cosmological Structures” (grant No. XDB09000000). National Astronomical Observatories, Chinese Academy of Sciences, and the Special Fund for Astronomy from the Ministry of Finance. Observations obtained with the Hale Telescope at Palomar Observatory were obtained as part of an agreement between the National Astronomical Observatories, Chinese Academy of Sciences, and the California Institute of Technology.