Different emitting components considered in our data analysis of AGNs hosting a black hole in its center. The inner hot corona (red) is responsible for continuum emission above 2 keV in the form of a power-law. The hard X-ray radiation illuminates each part of the inner disk and the reflection is self-consistently computed by our code, TITAN-NOAR. The reflected emission (magenta arrows) can originate from the outer disk (yellow) as well as from the distant torus (grey). The two-phase slab of warm corona (blue layer zone) and cold disk (yellow) is responsible for producing soft X-ray excess emission by up-scattering optical/UV seed photons (shown as yellow arrows) from the disk. Additional internal heating in this region assumed in our model is marked with curved green arrows.