Cumulative stellar sAM profiles for UGC9969, UGC6537, UGC10470, UGC8490, UGC10359, UGC11852, UGC10075, UGC8334, UGC3734, UGC11012, UGC5253, UGC2855, UGC6778, UGC11670, UGC9649, UGC12754, UGC5414, UGC4325, UGC4499, UGC1913, UGC9179, UGC11597, UGC4284, UGC7323, UGC9858, UGC2800, UGC5251, UGC7766, UGC3574 and UGC11914. All the profiles are shown until they reach their R_max. The dashed red line shows the last available radius in the hybrid RC of galaxies where extrapolation was necessary. The extrapolation remains below 50% of R_max for 13 out of 15 galaxies. The impact on j_★(< r) is limited, as these extrapolations only induce a median rise of 3%. The rise in j_★(< r) is between 36% and 38% for only two galaxies, between 11% and 17% for two other galaxies, and below 7% for all other galaxies.