ner_tags: O O O O O O O O O O B-Organization I-Organization I-Organization O O O B-Grant O O O O O O O O O B-Organization O O B-Grant B-Person O O O O B-Grant I-Grant B-Organization I-Organization I-Organization B-Grant I-Grant I-Grant I-Grant O O O B-Person I-Person I-Person O O O O O O O O O O O O O O O O O O O O O B-Telescope I-Telescope I-Telescope I-Telescope O O O O O B-Observatory I-Observatory I-Observatory I-Observatory O B-Observatory I-Observatory I-Observatory I-Observatory O O O O O B-Organization I-Organization I-Organization O O O O O B-Organization I-Organization I-Organization O O O O O O O O O O O B-Telescope I-Telescope O O O O B-Archive O O O O O B-Organization I-Organization I-Organization B-Observatory I-Observatory I-Observatory I-Observatory I-Observatory O O O O B-Telescope I-Telescope I-Telescope O O O O O O B-Organization I-Organization I-Organization B-Organization I-Organization I-Organization I-Organization O O O O B-Organization O O O O B-Telescope O O O O B-Organization O O O O O O O B-Organization I-Organization I-Organization O B-Organization I-Organization I-Organization O B-Organization I-Organization I-Organization I-Organization I-Organization O O O O O O O O B-Observatory I-Observatory I-Observatory O O O O O O O B-Telescope O O O O B-Organization I-Organization I-Organization O O O O B-Organization I-Organization I-Organization I-Organization I-Organization O O B-Location O O O O O O O O O O O B-Instrument O O O O B-Telescope B-Location B-Location B-Location B-Location O O B-Telescope I-Telescope O O O O O B-Organization I-Organization I-Organization B-Organization O B-Location O O B-Organization I-Organization I-Organization I-Organization I-Organization O O B-Organization I-Organization I-Organization I-Organization I-Organization I-Organization O B-Location O O B-Organization I-Organization I-Organization O O O O O O O O O O O O O O O O B-Telescope I-Telescope I-Telescope O O O O O B-Archive I-Archive I-Archive O O O O O O O O O B-Observatory I-Observatory I-Observatory O O O O O O O O O B-Organization I-Organization I-Organization I-Organization O B-Organization I-Organization I-Organization O O B-Organization I-Organization I-Organization I-Organization I-Organization O O O O O O O O O O O O B-Organization I-Organization I-Organization O O O O O O B-Location O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O
tokens: ACKNOWLEDGEMENTS This material is based upon work supported by the National Science Foundation under Grant No. 1411943. Part of the work presented herein is supported by NASA Grant No. NNX15AK92G. P.F.W. acknowledges funding through the Horizon 2020 European Research Council Consolidator Grant No. 683184. We thank the Stanislav S. Shabala as the referee for a constructive report that greatly improved the paper. This study is based on data taken with the Karl G. Jansky VLA that is operated by the National Radio Astronomy Observatory. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work is based, in part, on data collected at the Subaru Telescope and obtained from the SMOKA, which is operated by the Astronomy Data centre, National Astronomical Observatory of Japan; observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA; and data collected at UKIRT that is supported by NASA and operated under an agreement among the University of Hawaii, the University of Arizona, and Lockheed Martin Advanced Technology centre; operations are enabled through the cooperation of the East Asian Observatory. When the data reported here were acquired, UKIRT was operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the UK. This study is also based, in part, on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, and the Canada–France–Hawaii Telescope that is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawai’i. The scientific results reported in this article are based in part on observations made by the Chandra X-ray Observatory and data obtained from the Chandra Data Archive. The spectrographic data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. We wish to thank the indigenous Hawaiian community for allowing us to be guests on their sacred mountain, a privilege, without with, this work would not have been possible. We are most fortunate to be able to conduct observations from this site.