& Kuo11 & 0.08 & 0.084 - 0.30 & Kuo11\

[lcc]{} Name & Date of observation & Exposure time\
& & \[ks\]\
NGC 1194 & 2015-Feb-28 & 31\
NGC 1386 & 2013-Jul-19 & 21\
NGC 2273 & 2014-Mar-23 & 23\
NGC 2960 & 2013-May-10 & 21\
NGC 3079 & 2013-Nov-12 & 21\
NGC 3393 & 2013-Jan-28 & 15\
NGC 4388 & 2013-Dec-27 & 21\
IC 2560 & 2013-Jan-28, 2014-Jul-16 & 73\

### NGC 1194

NGC 1194 is a nearby Seyfert 1.9 galaxy. It hosts a circumnuclear maser disk which allowed a precise measurement of the BH mass of (6.5 $\pm$ 0.3) $\times$ 10$^7$ M$_{\odot}$ [@2011ApJ...727...20K]. Fitting the spectrum with an absorbed power law using a Galactic column returns an uncharacteristically hard photon index ($\Gamma$ $\sim$ 0.5) and leaves large residuals, in particular a prominent line feature at $\sim$ 6 - 7 keV and an excess between 10 and 30 keV ($\chi^2$/$\nu$ = 494/117). These are typical spectral signatures of an obscured AGN. A `plcabs` model (which accounts for obscuration) with two intrinsically narrow ($\sigma$ = 10 eV) Gaussian components for the lines at 6 - 7 keV returns a much better fit ($\chi^2$/$\nu$ = 186/112). The obscuration is in the 