Examples of mass modeled rotation curves in the case of the maximum stellar disk scenario (upper panel) and maximum stellar+gas disk (lower panel). The best-fit parameters are shown in the right column, and color codes are given in the legend of the plot, where ‘MM’ stands for dynamical mass-model profiles estimated using Bayesian inference, and ‘fid’ stands for fiducial profile derived from given photometric mass. This example favors the maximum stellar and baryonic disk scenario, upper and lower panels, respectively.