SED of the AGN component modeled as described in Sect. 2.2. The scale of the fluxes is arbitrary. The red lines correspond to a polar dust obscuration of the accretion disk emission with an SMC extinction curve, the dust emission is the sum of torus and polar dust emission at 500 K (red solid line) and 100 K (dashed line). The green line corresponds to a polar dust obscuration with a G04 extinction curve. All models are normalized to the same energy emitted by dust. The SED of the model without polar dust is shown as a blue short-dashed line, in this case the dust emission comes only from the dusty torus and the emission of accretion disk is unabsorbed along the line of sight.