SED fits using pure AGN models (magenta) of Seyfert nuclei: NGC 1365, NGC 4151, NGC 3081, and NGC 5643. High spatial resolution photometry is from Ramos Almeida et al. (2014b). Ground-based mid-IR spectroscopy of NGC 1365 is performed by Burtscher et al. (2013), NGC 3081 and NGC 4151 by Ramos Almeida et al. (2014b), and NGC 5643 by Hönig et al. (2010), respectively. Far-IR photometry of the nuclear region provided by NED or Herschel (Table 2) are plotted as upper limits of the AGN torus emission. Model parameters are given in Table 3.