tokens: We thank the anonymous referee, whose comments improved the clarity of the manuscript. M.N. acknowledges the support from the Vacation Scholarship program at the Centre for Astrophysics Supercomputing at Swinburne University of Technology. N.M.N. and G.G.K. acknowledge the support of the Australian Research Council through a Discovery Project DP170103470. S.K.P. acknowledges support through the Australian Government Research Training Program Scholarship. Parts of this research were supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project No. CE170100012. S.M. acknowledges support from European Research Council (ERC), Grant Agreement 278594-GasAroundGalaxies. C.W.C. and J.C.C. acknowledge the support from award 1517831 from the National Science Foundation. J.C.C. is also supported by National Science Foundation grant AST-1312686. This work made use of Python packages NumPy and SciPy (Oliphant 2007 ), Matplotlib (Hunter 2007 ), IPython (Pérez Granger 2007 ), tqdm (da Costa-Luis et al. 2018 ), and Numba (Lam et al. 2015 ) and of NASA’s Astrophysics Data System Bibliographic Services. Galaxy data presented here 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. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. Observations were supported by Swinburne Keck programs 2014A_W178E, 2014B_W018E, 2015_W018E, and 2016A_W056E. 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. Facility: Keck:II (ESI).
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