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Fig. 6.

image

Example of the SED fit for obscured AGN sources. The black dots indicate archival data, the error bars are shown in gray, the red pointers represent upper limits, and the purple crosses depict the mean flux in a 0.1 width logarithmic bin of frequency. The model fit (blue line) considers absorption at keV energies and in the optical band. The orange dashed line represents the unabsorbed emission from the accretion disk, the black dashed line indicates the optical absorbed disk emission, the green dashed line indicates the galactic template, the red dashed line depicts the emission from the dust belt, the cyan dashed line indicates the obscuring torus, and the purple dashed line indicates the absorbed corona emission. The gray vertical dashed line indicates the hydrogen Lyα frequency.

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