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tokens: We thank the technical staff of the University of Hawaii 2.2 m telescope, and Dan Birchall for his observing assistance. We recognize the significant cultural role of Maunakea within the indigenous Hawaiian community, and we appreciate the opportunity to conduct observations from this revered site. This work was supported in part by the Director, Office of Science, Office of High Energy Physics of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. We thank the Gordon Betty Moore Foundation for their continuing support. X.H. acknowledges the University of San Francisco (USF) Faculty Development Fund. Z.R. was supported in part by a USF Summer Undergraduate Research Fellowship. Support in France was provided by CNRS/IN2P3, CNRS/INSU, and PNC; L.P.N.H.E. acknowledges support from LABEX ILP, supported by French state funds managed by the ANR within the Investissements d’Avenir programme under reference ANR-11-IDEX-0004-02. N.C. is grateful to the LABEX Lyon Institute of Origins (ANR-10-LABX-0066) of the Université de Lyon for its financial support within the program “Investissements d’Avenir” (ANR-11-IDEX-0007) of the French government operated by the National Research Agency (ANR). Support in Germany was provided by the DFG through TRR33 “The Dark Universe;” and in China from Tsinghua University 985 grant and NSFC grant No 11173017. N.S. acknowledges the support from World Premier International Research Center Initiative (WPI), MEXT, Japan, and JSPS Program for Advancing Strategic International Networks to Accelerate the Circulation of Talented Researchers. This work is partially based on observations made with ESO Telescopes at the La Silla Paranal Observatory, Chile, under program 289.D-5035. Some results were obtained using resources and support from the National Energy Research Scientific Computing Center, supported by the Director, Office of Science, Office of Advanced Scientific Computing Research of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231.