tokens: We wish to thank our colleagues in the CANDELS, 3D-HST, and CLEAR collaborations for their intense work to make these data sets usable. The authors thank the anonymous referee for their constructive report, which improved the quality and clarity of this paper. We also thank them (and others) for productive conversations, comments, suggestions, and information, including Charlie Conroy, Romeel Davé, Sandy Faber, Kristian Finlator, Rob Kennicutt, Marcin Sawicki, Corentin Schreiber, and Sarah Wellons. V.E.C. acknowledges generous support from the Hagler Institute for Advanced Study at Texas AM University. This work benefited from generous support from George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University. This work is based on data obtained from the Hubble Space Telescope through program number GO 14227. Support for program number GO 14227 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.
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