Residual maps derived by computing the standard deviation along the wavelength axis of the residual cube, shown for all six halo models and the baryon-only model for the same galaxies shown in Fig. 6 and one more representative galaxy from our sample, for which we find mainly strong positive evidence for the DC14 model over the alternatives (except for Einasto and coreNFW). The titles of each panel show the log(𝒵) inferred from our MCMC fitting routine for the respective model. The Bayes Factor computed for each model against DC14 is shown in each panel, colour-coded as in Fig. 8.