Examples of the 3D disk-halo decomposition for the two galaxies from the sample. The solid black line represents the circular velocity v_c(r) corrected for pressure support. The solid green curve represents the RC of the DM component. The solid orange and blue curves represent the disk and cold gas components, respectively. The light shaded regions show the 95% CI. The dotted brown line represents the stellar component measured using the multi-Gaussian expansion modelling of resolved stellar mass maps obtained from pixel-by-pixel SED fitting, while the dash-dotted green curve shows the DM component obtained independently from a 1D disk–halo decomposition. All velocities are intrinsic, i.e. corrected for inclination and instrumental effects, including seeing (PSF). The black dotted line shows the physical extent of a MUSE spaxel.