Modeling time delays from two reprocessors in active galactic nuclei

Open Access

Fig. 5.

Comparison between disk response function and disk plus BLR response function for different BLR profiles (Gaussian, half-Gaussian, and exponential; see Fig. 2), and 30% BLR contribution is used. Parameters: black hole mass 10⁸ M_⊙, Eddington ratio = 1.0, L_X = 10⁴⁰ erg s⁻¹, height h = 5r_g, viewing angle i = 30 degrees.

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