Stellar mass TFR for the MAGIC group sample, using the rotation velocity. The black circles correspond to galaxies fulfilling the strict conditions (S/N > 40 and R_eff/FWHM > 0.5), whereas circles without contours indicate additional galaxies with more relaxed conditions (S/N > 30 and R_eff/FWHM > 0.25). Small squares show all other galaxies on the main sequence with velocity flags larger than or equal to 2. The color indicates the values of V_r22/σ. The three horizontal dashed lines indicate the threshold in mass used. For galaxies in the kinematic sample, we also identify bulge-dominated galaxies (double circles) and problematic AGN (circled stars) that are discarded from the analysis of the final sample.