Rotation velocity (upper panels, pink) and velocity dispersion profiles (bottom panels, green) for the ALPAKA galaxies classified as disks. The circles show the location of the rings used for fitting the data with ^3DBAROLO and they can be considered independent from each other. The dashed vertical lines show the location of the optical/UV effective radius R_e for ALPAKA galaxies with HST data and with R_e comparable to or smaller than the extent of the CO/[CI] emission.