Best fit with the DMD and NFW models for some of the galaxies in our sample: CVnIdwA (a), DDO43 (b), DDO46 (c), DDO47 (d), DDO50 (e), and DDO52 (f). The circular velocity due to the stellar and gas components is also shown. For comparison, we report in some cases the asymmetric drift-corrected rotation curves measured by Iorio et al. (2017, Iorio+17) and Mancera Piña et al. (2022, MP+22). For the other fits of the rotation curves, see Figs. B.1 and B.2.