Stellar mass TFR for the MAGIC final kinematic sample, using the rotation velocity. The black dots indicate galaxies used for the reference subsample with stellar masses above 10⁹ M_⊙, whereas gray dots indicate the other galaxies for information. The black line corresponds to the fit to the MAGIC group sample with a free slope and the intrinsic scatter is represented with the gray shaded area. The parameters of this fit are indicated in the figure. Colored dotted-dashed lines correspond to fits on other samples, with an offset of −0.15 dex for the correction of the stellar mass. The slopes of these fits are used to perform additional fits of the smTFR on the MAGIC group sample. The corresponding fits are shown with continuous lines having the same colors as the samples used as reference for the slope.