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tokens: ACKNOWLEDGEMENTS ADM holds an Australian Research Council (ARC) Future Fellowship (FT160100206), and acknowledges support from ARC Discovery Project DP150103294. We would like to thank the anonymous referee for their thorough reading of this manuscript and for their helpful suggestions for improvement. This paper is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada–France–Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. This paper is also based, in part, on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil). These observations were obtained via programmes GN-2014B-Q-26 and GN-2015B-Q-17.