Quality of the AGN subtraction with Budda: difference between host galaxy in synthetic image and Budda fit in magnitudes (left), same for the bulge component (right), as a function of the fitted AGN (left) or bulge (right) luminosity fraction. Positive errors indicate that there is more flux in the model than in the original component, e.g. that the host galaxy or bulge resp. is overestimated; squares indicate disk-dominated galaxies; circles bulge-dominated galaxies, and diamonds barred galaxies. In the right panel, we mark trends by the mean and standard deviation of the data points in bins of 0.2 of the AGN/bulge fraction.