tokens: We acknowledge the support from a 985 project at Peking University. L.J., S.C., and E.E. also acknowledge the support from NASA through awards issued by STScI ( HST PID: 11149,12329,12616) and by JPL/Caltech ( Spitzer PID: 40026,70094). We would like to thank R. Ryan for his advice on IRAC photometry and using iGALFIT . We also thank J. Rhoads and Z. Zheng for their insightful comments, and thank P. Madau and P. A. Oesch for providing us with the data used for Figures 10 and 12 . Facilities: HST (NICMOS,WFC3) , Spitzer (IRAC) , Subaru (Suprime-Cam) .
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