tokens: We thank Peter Stetson for a copy of DAOPHOT as well as his helpful engagement on its usage. We also thank C. Gallart and M. Monelli of the LCID team for a copy of their IC 1613 photometric catalog for comparison to our own. We also thank Richard Kron for helpful comments in this research and preparation of this manuscript, Julia Kollmeier for helpful conversations, and Laura Sturch for the preparation of IMACS imaging. In addition, we thank the anonymous referee for numerous constructive suggestions. Authors M.G.L. and I.S.J. were supported by the National Research Foundation of Korea (NRF) grant funded by the Korea Government (MSIP) No. 2012R1A4A1028713. Support for program #13691 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, Inc., under NASA contract NAS 5-26555. 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 paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. We thank the Carnegie Institution for its continued support of this program over the past 30 years. Facilities: HST (ACS/WFC , WFC3-IR) , Magellan-Baade (IMACS) . Software: DAOPHOT (Stetson 1987 ), ALLFRAME (Stetson 1994 ), Tiny Tim (Krist et al. 2011 ).
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