given that phenomenological models point towards a highly obscured, reflection dominated source, and that the best fit in a physical and self-consistent model is represented by a back-scattered radiation dominated `MYTorus` model, we conclude that NGC 1194 is a Compton-thick AGN, with the column density $N_{\rm H}$ = 1.4$^{+ 0.3}_{- 0.2}$ $\times$ 10$^{24}$ cm$^{-2}$, consistent with the one reported by @2008ApJ...686L..13G. We note that, according to the best fit model, reflection dominates below $\sim$10 keV only. Best fit spectral parameters are given in Table \[table:table\].

[l c c c c c c c c ]{} Parameter & NGC 1194 & NGC 1386 & NGC 2273 & NGC 2960 & NGC 3079 & NGC 3393 & NGC 4388 & IC 2560\
Best fit model & MYT D & T & T & MYT & MYT & T & MYT D & T\
$\chi^2$/$\nu$ & 113/112 & 32/25 & 123/113 & 6/5 & 189/152 & 49/69 & 693/681 & 125/104\
$\Gamma$ & 1.59 $\pm$ 0.15 & &gt; 2.6 & 2.1 $\pm$ 0.1 & 1.9 (f) & 1.8 $\pm$ 0.2 & 1.8 $\pm$ 0.2 & 1.65 $\pm$ 0.08 & 2.7 $\pm$ 0.1\
$N_{\rm H}$ \[cm$^{-2}$\] & 1.4$^{+ 0.3}_{- 0.2}$ $\times$ 10$^{24}$ & (5 