Effect of bulge prominence on the AGN fraction (f_AGN) for strongly barred (solid red), weakly barred (dashed navy), and unbarred (dotted teal) disk galaxies. Overall, f_AGN increases in each bar strength category with bulge prominence. At lower bulge prominences, f_AGN increases in each bulge bin with bar strength; however, the difference between f_AGN in strongly and weakly barred galaxies disappears by B ≈ 0.48, and the difference between all three bar categories disappears around B ≈ 0.6. The shaded regions show the 1σ uncertainties.