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tokens: We are grateful to the entire Gaia collaboration for providing data and assistance which made this project possible. We congratulate them on their tremendous achievement to date. Support for this work was provided by the National Aeronautics and Space Administration (NASA) through programs GO-12879, 13334, 13335, 13344, 13571, 13678, 13686, 13928, 13929, 14062, 14394, 14648, 14868 from the Space Telescope Science Institute (STScI), which is operated by AURA, Inc., under NASA contract NAS 5-26555. B.B. and M.G.L. are indebted to the Italian Space Agency (ASI) for their continuing support through contract 2014-025-R.1.2015 to INAF, and to R. Morbidelli (INAF) and R. Messineo (ALTEC S.p.A, Torino) of the Italian Data Processing Center (DPCT) for their help with the Gaia data. A.V.F.’s group at UC Berkeley is also grateful for financial assistance from the TABASGO Foundation, the Christopher R. Redlich Fund, and the Miller Institute for Basic Research in Science (UC Berkeley). S.C. and A.G.R. gratefully acknowledge support by the Munich Institute for Astro- and Particle Physics (MIAPP) of the DFG cluster of excellence “Origin and Structure of the Universe.” This research is based primarily on observations with the NASA/ESA Hubble Space Telescope , obtained at STScI, which is operated by AURA, Inc., under NASA contract NAS 5-26555. This publication makes use of data products from the Wide-field Infrared Survey Explorer (WISE) , which is a joint project of the University of California (Los Angeles) and the Jet Propulsion Laboratory/California Institute of Technology, funded by NASA. It has also made use of the SIMBAD database, operated at CDS, Strasbourg, France. Research at Lick Observatory is partially supported by a generous gift from Google. The HST data used in this paper are available at the MAST archive doi: 10.17909/T9G40B .