Detailed multi-wavelength modelling of the dark GRB 140713A and its host galaxy

We greatly appreciate the support from the WSRT and AMI staff in their help with scheduling and obtaining these observations. The WSRT is operated by ASTRON (Netherlands Institute for Radio Astronomy) with support from the Netherlands foundation for Scientific Research. The AMI arrays are supported by the University of Cambridge and the STFC. Some of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration (NASA); the Observatory was made possible by the generous financial support of the W.M. Keck Foundation. The Nordic Optical Telescope is operated on the island of La Palma by the Nordic Optical Telescope Scientific Association in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. ABH is supported by a Science and Technology Facilities Council (STFC) studentship. RLCS, KW and NRT acknowledge support from STFC. GA acknowledges the support of the European Research Council Advanced Grant 267697 ‘4 Pi Sky: Extreme Astrophysics with Revolutionary Radio Telescopes’. GA is the recipient of an Australian Research Council Discovery Early Career Researcher Award (project number DE180100346) funded by the Australian Government.