tokens: ACKNOWLEDGEMENTS The groundwork for this paper began as an MPhys project completed by Alison Young and Jemma Holloway at the University of Exeter. We are grateful to David Acreman for assistance with running TORUS. We would also like to thank Nathan Mayne and Tim Naylor for helpful discussions regarding SED fitting and photometry. Finally, we thank the anonymous referee and Michael Dunham for comments that helped to improve the paper. Some figures were produced using the publically available SPLASH visualization software (Price 2007 ). This work was supported by the European Research Council under the European Commission’s Seventh Framework Programme (FP7/2007-2013 Grant Agreement No. 339248). The calculations discussed in this paper were performed on the University of Exeter Supercomputer, a DiRAC Facility jointly funded by Science and Technology Facilities Council (STFC), the Large Facilities Capital Fund of Department for Business Innovation Skills (BIS), and the University of Exeter. This work used the DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment is funded by BIS National E-Infrastructure capital grant ST/K000373/1 and STFC DiRAC Operations grant ST/K0003259/1. DiRAC is part of the National E-Infrastructure. The JCMT has historically been operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the United Kingdom, the National Research Council of Canada and the Netherlands Organisation for Scientific Research. Additional funds for the construction of SCUBA-2 were provided by the Canada Foundation for Innovation. Chris Mowat is supported by an STFC studentship. This research has made use of NASA’s Astrophysics Data System. This research used the services of the Canadian Advanced Network for Astronomy Research (CANFAR), which is supported by CANARIE, Compute Canada, University of Victoria, the National Research Council of Canada, and the Canadian Space Agency. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency. Starlink software (Currie et al. 2014 ) is supported by the East Asian Observatory. matplotlib is a 2D graphics package used for Python for application development, interactive scripting, and publication-quality image generation across user interfaces and operating systems. This research made use of aplpy (Robitaille Bressert 2012 ), an open-source plotting package for Python hosted at http://aplpy.github.com . Herschel is an ESA space observatory with science instruments provided by European-led principal investigator consortia and with important participation from NASA. This research has made use of data from the Herschel Gould Belt survey (HGBS) project ( http://gouldbelt-herschel.cea.fr ). The HGBS is a Herschel Key Programme jointly carried out by SPIRE Specialist Astronomy Group 3 (SAG 3), scientists of several institutes in the PACS Consortium (CEA Saclay, INAF-IFSI Rome and INAF-Arcetri, KU Leuven, MPIA Heidelberg), and scientists of the Herschel Science Center (HSC). The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.
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