Dependence of the multiplicative bias on S/N_KSB and comparison between the S/N_KSB correction from S10 (shown in blue) and the new correction presented in Eq. (13). The red and black dashed lines show the correction for the two shear components. We binned the galaxies according to their S/N_KSB and computed the bias for each bin separately. We include no S/N_flux cuts here but note that the inclusion of a S/N_flux >  10 cut changes the results only slightly.