emission (we require the emission to be at least 5 times the RMS) of the high velocity maser features, we find that the innermost radius is $\sim$ 0.034 pc, consistent with @2011ApJ...727...20K, but that the outermost radius is $\sim$ 0.2 pc. We adopt these values in the following analysis. A `MYTorus` model cannot account for the line emission, and gives an unacceptable fit ($\chi^2$/$\nu$ = 267/113). Its decoupled mode provides an acceptable fit ($\chi^2$/$\nu$ = 131/111), pointing towards a back-scattered, reflection dominated AGN. However, the best fit is found with the `Torus` model, where the source is heavily Compton-thick and a lower limit on the column density is found ($N_{\rm H}$ &gt; 7.3 $\times$ 10$^{24}$ cm$^{-2}$), consistently with @2005MNRAS.356..295G and @2009PASJ...61S.317A. `Torus` spectral parameters are found in Table \[table:table\], while the best fit model is shown in Figure \[fig:subfig3\].

### NGC 2960

The central black hole mass of the spiral megamaser galaxy NGC 2960 (Mrk 1419) as reported by @2011ApJ...727...20K is (1.16 $\pm$ 0.05) $\times$ 10$^7$ M$_{\odot}$. NGC 2960 is very faint, and a 21 ks *NuSTAR* snapshot resulted in poor quality data which prevented us from significantly constraining spectral parameters. The fitting procedure in XSPEC was carried out using 