Impact of AGN parameters on the SED in face-on (top) and edge-on (bottom) view. We vary the inner radius rin for models a) without and b) with a disk; c) the optical depth of the disk midplane τV,mid; d) the volume fraction of the clouds η; and e) the optical depth of the clouds τV,cl. Unless otherwise specified rin = 0.25 pc, τV,mid = 100, η = 38.5%, and τV,cl = 4.5.
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