Oral title: The mid-infrared emitting structure of the BASS AGN

Oral abstract: Here we address whether in the BASS AGN sample there is evidence for changes in the mid-infrared (MIR) 
spectral energy distribution (SED) with the AGN fundamental parameters such as luminosity, Eddington ratio or X-ray 
column density. Such changes are expected based on the result results indicating a decreasing obscuration with 
increasing Eddington ratio.
Indeed, we find possible corresponding change in the MIR SED, as well as the expected reddening with increasing 
obscuration and a bluening with increasing luminosity. All these results will be briefly discussed.