Same as Fig. 6, but here we distinguish between galaxies with stellar masses below 10⁹ M_⊙ and above 10¹⁰ M_⊙. The numbers indicated in each panel correspond to the sample sizes used to generate the histograms. Values in parentheses denote the KS test p_KS values. The results suggest that low-mass galaxies exhibit a more uniform distribution of BH–galaxy misalignment angles (characterized by p_KS > 0.05). Note that only good cases are shown, assuming a uniform perturbation of the BH spin of 30°, with no morphological distinction between spheroidal and disk galaxies.