Comparison of the time lags induced by the Milky Way and by AGN dust prescription for the case of a uniform dusty torus and a uniform flared disk. The plots showthe time lag as a function of wavelength for different viewing angles: the magenta dots denote θ = 79.9^∘ , and the red dots θ = 71.0^∘ , which represents a type 2 view. The black dots show θ = 61.64^∘ , a view close to the torus horizon. Type 1 views are shown in green (θ = 51.3^∘ ), blue (θ = 39.19^∘ ), and cyan (θ = 28.9^∘).