tokens: This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00988.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. We are grateful to the European ALMA Regional Centres, particularly those in Garching and Manchester, for their dedicated end-to-end support of data associated with this paper. We have also received immense support from the National Radio Astronomy Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work is also based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 094.A-0959 (PI: Hamer). We also present observations made with the NASA/ESA Hubble Space Telescope , obtained from the data archive at the Space Telescope Science Institute (STScI). STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. G.R.T. thanks E.S.T. and A.S.T. for educating him on nature’s many sources of uplift. G.R.T. also acknowledges support from the National Aeronautics and Space Administration (NASA) through Chandra Award Number GO7-8128X as well as Einstein Postdoctoral Fellowship Award Number PF-150128, issued by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060. B.J.W., S.W.R., J.A.Z., P.E.J.N., R.P.K., W.R.F., C.J., and Y.S. also acknowledge the financial support of NASA contract NAS8-03060 ( Chandra X-ray Center). F.C. acknowledges the European Research Council for the Advanced Grant Program # 267399-Momentum. M.G. is supported by NASA through Einstein Postdoctoral Fellowship Award Number PF5-160137, as well as Chandra grant GO7-18121X. The work of S.A.B., C.P.O., and B.R.M. was supported by a generous grant from the Natural Sciences and Engineering Research Council of Canada. H.R.R. and T.A.D. acknowledge support from a Science and Technology Facilities Council (STFC) Ernest Rutherford Fellowship. A.C.E. acknowledges support from STFC grant ST/P00541/1. A.C.F. acknowledges support from ERC Advanced Grant “Feedback.” M.N.B. acknowledges funding from the STFC. Basic research in radio astronomy at the Naval Research Laboratory is supported by 6.1 Base funding. This research made use of Astropy , 39 39 http://www.astropy.org/ a community-developed core Python package for Astronomy (The Astropy Collaboration et al. 2013 , 2018 ). Some MUSE data reduction and analysis was conducted on Hydra, the Smithsonian Institution’s High Performance Cluster (SI/HPC). Facilities: CXO (ACIS-S) , HST (ACS , NICMOS) , VLT: Yepun . Software : Astropy (The Astropy Collaboration et al. 2013 , 2018 ), CASA (McMullin et al. 2007 ), CIAO (Fruscione et al. 2006 ), IPython (Perez Granger 2007 ), Matplotlib (Hunter 2007 ), NumPy (van der Walt et al. 2011 ), PySpecKit (Ginsburg Mirocha 2011 ), scipy (Jones et al. 2001 ). DOI-linked software repository for this paper .
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