From left to right: stellar, gas, and baryonic j − M relations for our sample of galaxies. In all the panels the circles represent the observed galaxies, while the dashed black line and grey region show, respectively, the best-fitting relations and their perpendicular intrinsic scatter. The three relations are well fitted by unbroken power-laws: The best-fitting relations are shown for each panel (see Table 2). We remind the reader that each panel includes only the galaxies with convergent j_*, j_gas, and j_bar profile, respectively, so the galaxies shown in one panel are not necessarily the same as in the other panels.