tokens: H.D. acknowledges financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) under the 2014 Ramón y Cajal program MINECO RYC-2014-15686. J.L.W. acknowledges support from an STFC Ernest Rutherford Fellowship. D.R. acknowledges support from the National Science Foundation under grant number AST-1614213. G.D.Z. acknowledges support from ASI/INAF agreement n. 2014-024-R.1. We pay special thanks to the useful feedback provided on the draft version of this work to D. Farrah, J. Greenslade, M. J. Michalowski, and I. Valtchanov. This research has made use of data from Her MES project ( http://hermes.sussex.ac.uk/ ). Her MES is a Herschel Key Programme utilizing Guaranteed Time from the SPIRE instrument team, ESAC scientists and a mission scientist. The H -ATLAS is a project with Herschel , which is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. The H -ATLAS website is http://www.h-atlas.org . US participants in H -ATLAS acknowledge support from NASA through a contract from JPL. This publication is based on data acquired with the Atacama Pathfinder Experiment (APEX). APEX is a collaboration between the Max-Planck-Institut für Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. Based on observations made with APEX under European Southern Observatory program E-191.A-0748 and Max Planck Institute (MPI) programs M-090.F-0025-2012, M-091.F-0021-2013 and M-092.F-0015-2013. Facilities: APEX , Herschel .
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