Fig. 6.

SED assuming B = 600 G and Lp/Le = 100. The number of cloud impacts, Nevents, is determined by adjusting the model to match the observed total gamma luminosity. The gamma absorption is produced by the UV photons of the BLR and the optical photons from the accretion disk. The regions contained in the dashed rectangles are expanded in Figs. 7 and 8.
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