tokens: Based on observations obtained at the Gemini Observatory (processed using the Gemini iraf package), which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnologa e Innovacin Productiva (Argentina), and Ministrio da Cincia, Tecnologia e Inovao (Brazil), and observations collected at the Centro Astronmico Hispano Alemn (CAHA), operated jointly by the Max-Planck Institut fr Astronomie and the Instituto de Astrofisica de Andalucia (CSIC). VVG acknowledges the Russian Science Foundation grant 14-12-01096. JM acknowledges funding from a Royal Society Science Foundation Ireland University Research Fellowship (No. 14/RS-URF/3219). AYK acknowledges support from the National Research Foundation (NRF) of South Africa and the Russian Foundation for Basic Research grant 16-02-00148. TJH is funded by an Imperial College Junior Research Fellowship. This research was supported by the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., on behalf of the international Gemini partnership of Argentina, Brazil, Canada, Chile, and the United States of America, and has made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, the SIMBAD data base and the VizieR catalogue access tool, both operated at CDS, Strasbourg, France.
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