Left: as in Fig. 11, but for mass accretion rate and stellar mass. Differences between the two methods affect the and M_* directions. Fits to the black and red distributions and black and blue distributions are shown as solid red and blue lines, respectively. Right: Distribution of the dispersion from the individual best-fitting M_acc − M_* relation considering the total sample with the 2 T_eff (red) and the single T_eff (blue) modeling for the spotted source. The dispersion of the distributions is labeled in the panel.