Luminosity of the central source L_ν(θ) is presented for an inclination of θ = 75°, defined in Equation (2). The shape of the spectra is determined by α_ox = −1.5. For all the inclination angles, the shape of the spectra remains unchanged, whereas the total luminosities vary with f(θ). The material around the AGN is solely heated by the radiation from the central source.