tokens: This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00634.S and ADS/JAO.ALMA#2011.0.00004.SV. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work is partially based on observations carried out with the IRAM IRAM 30 m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). The work of M.G. and A.K.L. is partially supported by the National Science Foundation under grant nos. 1615105, 1615109, and 1653300. E.S. acknowledges financial support to the DAGAL network from the People Programme (Marie Curie Actions) of the European Union’s Seventh Framework Programme FP7/2007–2013/under REA grant agreement no. PITN-GA-2011-289313. A.H. acknowledges support from the Centre National d’Etudes Spatiales (CNES). A.U. acknowledges support from Spanish MINECO grants ESP2015-68964 and AYA2016-79006. E.R. is supported by a Discovery Grant from NSERC Canada. F.B. acknowledges funding from the European Unions Horizon 2020 research and innovation programme (grant agreement no. 726384—EMPIRE) This paper made use of the NASA Astrophysics Data Abstract service, AstroPy, the IDL Astronomy User’s Library, CASA, and the NASA Extragalactic Database. M.G. and A.K.L. gratefully acknowledge helpful discussions with Todd Thompson and the OSU galaxy and ISM discussion groups. Diane Cormier is supported by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement no. 702622. M.J.J.-D. and F.B. acknowledge support from DFG grant BI 1546/1-1. E.O. is supported by grant AST-7173949 from the National Science Foundation.
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