ner_tags: O O O O O O O O B-Telescope I-Telescope O O O O O B-Observatory I-Observatory I-Observatory I-Observatory I-Observatory B-Person O B-Person O O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization I-Organization B-Grant I-Grant I-Grant I-Grant B-Person O O O O B-Organization I-Organization I-Organization B-Organization B-Person O O O B-Organization B-Grant I-Grant I-Grant I-Grant O O O O O O O O O O B-Archive I-Archive I-Archive I-Archive O O O O O B-Organization I-Organization I-Organization B-Organization I-Organization I-Organization I-Organization O O O B-Organization O O O O O O O B-Person I-Person B-Person I-Person B-Person I-Person B-Person I-Person O B-Person I-Person O O O O O O O O O O O O O O O O O O O B-Person I-Person O O O O O O O O
tokens: This paper is based on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. GM and II are supported by Japan Society for the Promotion of Science KAKENHI Grant number: 24244018. GM acknowledges support by the Swedish Research Council (Vetenskapsrådet). AKI is supported by JSPS KAKENHI Grant number: 26287034. A part of this research 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 NASA. We extend a warm thank you to Yuichi Matsuda, Katsuki Kousai, Elisabeta Lusso, Cristian Saez, and Alice Shapley for providing us with their spectra, and with some clarifications on their work and helpful advice. We also thank Andrea Grazian for useful suggestions and comments on this work.