the Cash statistic [@1979ApJ...228..939C], but we report the reduced $\chi^2$ for direct comparison with other sources. Using a default `MYTorus` model and fixing the photon index $\Gamma$ = 1.9 (Figure \[fig:subfig4\]), the fit returns an obscured, but Compton-thin, source ($N_{\rm H}$ = 5$^{+ 4}_{- 3}$ $\times$ 10$^{23}$ cm$^{-2}$), marginally consistent with @2008ApJ...686L..13G . Results are listed in Table \[table:table\].

### NGC 3079

The low ionization nuclear emission-line region (LINER) galaxy NGC 3079 presents a thick, flared, probably star forming and self-gravitating maser disk [@2005ApJ...618..618K]. The disk outer radius is indeed beyond the sphere of influence radius of the central mass, which is 2.4$^{+ 2.4}_{- 1.2}$ $\times$ 10$^6$ M$_{\odot}$ [@2013ApJ...764..184M]. Either `Torus` ($\chi^2$/$\nu$ = 193/152) or `MYTorus` ($\chi^2$/$\nu$ = 189/152), both with a scattered power law dominating below 5 keV, give similar results. Using a decoupled `MYTorus` model ($\chi^2$/$\nu$ = 189/150), the back-scattered contribution vanishes, confirming that the source is dominated by reflection below 10 keV. We therefore choose the coupled `MYTorus` model as the best fit (Figure \[fig:subfig5\]), and conclude that NGC 3079 is transmission dominated with a column density of $N_{\rm H}$ = (2.5 $\pm$ 0.3) $\times$ 10$^{24}$ cm$^{-2}$ (see Table \[table:table\] for other parameters). This result is in 