\begin{table}%t1
\caption{\label{tab:fluxes}Observed properties of the sample.}
  %\centerline
 $$
  \begin{tabular}{lccccr@{~~~}l@{~~~}r@{$\;\pm\;$}lr@{~~~}l@{~~~}r@{$\;\pm\;$}lcr}
    \hline\hline
    Target                   & Sy  & $z$     &\lognh & $r_0$  & \multicolumn{4}{c}{Secondary filter flux}              & \multicolumn{4}{c}{Primary filter flux}              & log $\lambda L_{\lambda}$  & log \lx            \\
                             &     &         & cm$^{-2}$ & pc  & Name & $\lambda_{\rm C}$  & \multicolumn{2}{c}{mJy}          & Name & $\lambda_{\rm C}$        & \multicolumn{2}{c}{mJy} & erg s$^{-1}$               & erg s$^{-1}$ \\
      (1)                    & (2) &  (3)    &  (4)   & (5)     & \multicolumn{2}{c}{(6)}  &  \multicolumn{2}{c}{(7)} &  \multicolumn{2}{c}{(8)}   &  \multicolumn{2}{c}{(9)} &         (10)              &         (11)                \\
    \hline\\[-3.2mm]
    {\it NGC~1068}           & {\it 1h} & {\it 14.4$^d$}&{\it $>$25} &{\it 25} & \multicolumn{4}{c}{--}                     & \multicolumn{2}{c}{$\approx${\it 12 $\mu$m}$^{*}$}& \multicolumn{2}{c}{{\it $\sim$9500}}& {\it 43.80$\;\pm\;$0.02}        &    {\it 43.4$\;\pm\;$0.3}     \\ 
    Swift~J0138.6--4001      & 2   & 0.0252  & 23.7   & 175    & SIV  & 10.49              & 20&3                     & PAH2 & 11.25              & 34&3                     &  43.10$\;\pm\;$0.04             &        43.6$\;\pm\;$0.3        \\
    Swift~J0601.9--8636      & 2   & 0.0062  & 24.0   & 45     & PAH2 & 11.25              & 13&4                     & NEII\_2 & 13.04              & 72&15                     &  42.11$\;\pm\;$0.08             &        41.9$\;\pm\;$0.3        \\
    ESO~209--G012            & 1.5 & 0.0405  & $<$22  & 280    & PAH2 & 11.25              & 162&10                   & NEII & 12.81              & 188&26                   &  44.22$\;\pm\;$0.06             &        43.7$\;\pm\;$0.2        \\
    NGC~3081                 & 1h  & 0.0078  & 23.8   & 55     & PAH2 & 11.25              & 161&11                   & NEII\_2 &  13.04             & 138&11                   &  42.64$\;\pm\;$0.03             &        42.6$\;\pm\;$0.3        \\
    ESO~263--G013            & 2   & 0.0333  & 23.6   & 225    & SIC  & 11.85              & 45&4                     & NEII & 12.81              & 46&3                     &  43.42$\;\pm\;$0.02             &        43.3$\;\pm\;$0.4        \\
    NGC~3281                 & 2   & 0.0107  & 24.3   & 75     & PAH2 & 11.25              & 481&24                  & NEII\_2 &  13.04             & 1016&52                   &  43.76$\;\pm\;$0.02             &        43.3$\;\pm\;$0.2        \\
    NGC~3393                 & 2   & 0.0125  & 24.2   & 90     & SIV  & 10.49              & 36&2                     & NEII\_2 & 13.04           & 94&5                     &  42.90$\;\pm\;$0.02             &        43.0$\;\pm\;$0.3        \\
    NGC~4388                 & 1h  & 16.7$^d$& 23.4   & 30     & PAH2 & 11.25              & 147&11                   & NEII\_2 & 13.04              & 375&28                   &  42.45$\;\pm\;$0.03             &        42.2$\;\pm\;$0.3        \\
    IC~3639                  & 1h  & 0.0109  & $>$25  & 75     & PAH2 & 11.25              & 326&17                   & NEII\_2 & 13.04              & 542&29                   &  43.51$\;\pm\;$0.02             &        43.6$\;\pm\;$0.5        \\
    ESO~323--G032            & 1.9 & 0.0160  & --     & 110    & \multicolumn{4}{c}{--}                               & PAH2 & 11.25              & 61&6                     &  42.96$\;\pm\;$0.04             &        42.4$\;\pm\;$0.4        \\
    NGC~4992                 & 2   & 0.0251  & 23.7   & 175    & PAH1 & 8.59               & 61&6                     & NEII & 12.81              & 71&4                     &  43.36$\;\pm\;$0.02             &        43.2$\;\pm\;$0.3        \\
    NGC~5728                 & 1.9 & 0.0094  & 24.3   & 65     & \multicolumn{4}{c}{--}                               & NEII\_2 & 13.04           & 123&10                   &  42.60$\;\pm\;$0.03             &        42.8$\;\pm\;$0.3        \\
    ESO~138--G001            & 2   & 0.0091  & $>$24.3& 65     & PAH2 & 11.25              & 776&40                   & NEII\_2 &  13.04             & 862&45                   &  43.54$\;\pm\;$0.02             &        43.0$\;\pm\;$0.3        \\
    NGC~6300                 & 2   & 0.0037  & 23.3   & 25     & PAH2 & 11.25              & 278&14                   & NEII\_2 &  13.04             & 727&38                   &  42.69$\;\pm\;$0.02             &        42.3$\;\pm\;$0.3        \\
    ESO~103--G035            & 2   & 0.0133  & 23.3   & 95     & SIV  & 10.49              & 243&15                   & NEII\_2 & 13.04           & 622&49                   &  43.74$\;\pm\;$0.03             &        43.4$\;\pm\;$0.2        \\
    NGC~6814                 & 1.5 & 0.0052  & $<$20.5& 35     & PAH2 & 11.25              & 99&6                     & NEII\_2 & 13.04              & 96&6                     &  42.07$\;\pm\;$0.02             &        42.1$\;\pm\;$0.4        \\
    \hline
  \end{tabular}$$
\par
\medskip
$^d$ Distances in Mpc. $^{*}$ For NGC~1068, the fluxes are from high angular resolution (0\farcs2--0\farcs4) Keck and Subaru studies \citep{mason06, tomono01} at slightly-differing wavelengths. All values for this source are written in italic font simply to draw attention to the fact that the observations are entirely drawn from other publications. See Appendix.
\end{table}