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We investigate the most general version of the external Comp t n model for the gamma-ray production by considering 3-dimensional, inverse Compton ee pair cascades initiated by leptons which interact with the thermal radiation from an accretion disk. The spectral properties and the time evolution of the GeV-TeV gamma-ray emission produc e in such cascade for different locations of the observer in respect to the direction of the j et are studied in detail. We compare the results of calculations with the GeV-TeV observations o f AGNs viewed at small and large inclination angles, taking as an example the parameters of t he two famous sources Cen A and 3C 279.

Time dependent production of gamma-rays in the inverse Compton $e^+e^-$ pair cascades in AGNs.