\begin{table}%t1
\caption{\label{tab:scales}Characteristics of our type 1 AGN mid-IR spectroscopic sample.}
%\centering
\par
\begin{tabular}{l c c c  c c c c  c c c }
\hline\hline \noalign{\smallskip}
Object           & Type\tablefootmark{a}  & $z$      & $D_L$\tablefootmark{b} & \multicolumn{4}{c}{log Luminosities (erg/s)} & \multicolumn{3}{c}{Object scales}  \\
                 &           &        & (Mpc)     & $\Lx$ ($\nh$)\tablefootmark{c} & $\Lv$\tablefootmark{d} & $\Loiii$\tablefootmark{e} & $\Lm$\tablefootmark{f} & $\rsub$\tablefootmark{g} (pc) & 8~$\micron$ (pc)\tablefootmark{h} & res. ($\rsub$) \\ 
                 \hline
         NGC~3227 &      S1.5 & 0.0049 & ~20.4     & 42.40 (22.80) & 42.20 & 40.51 & 42.63         & 0.014 & ~24.2 & 1680 \\
         NGC~3783 &      S1.5 & 0.0108 & ~44.7     & 43.19 (22.47) & 42.98 & 41.30 & 43.57         & 0.035 & ~52.5 & 1482 \\
         NGC~4593 &      S1.0 & 0.0101 & ~42.0     & 42.89 (20.30) & 42.88 & 40.69 & 43.18         & 0.032 & ~49.5 & 1560 \\
     ESO~323--G77 &      S1.2 & 0.0159 & ~66.3     & 42.76 (23.25) & 43.91 & 41.05 & 43.75         & 0.104 & ~77.1 & ~741 \\
   MCG--6--30--15 &      S1.5 & 0.0087 & ~35.8     & 42.86 (21.67) & 43.41 & 40.36 & 43.09         & 0.058 & ~42.3 & ~727 \\
         IC~4329A &      S1.2 & 0.0170 & ~70.5     & 43.87 (21.65) & 44.11 & 41.21 & 44.20         & 0.131 & ~82.0 & ~625 \\
         MARK~509 &      S1.5 & 0.0335 & 141~~     & 43.94 (20.70) & 44.01 & 42.29 & 44.25         & 0.116 & 158~~ & 1365 \\
         NGC~7213 &     S1.5L & 0.0051 & ~21.2     & 42.33 (20.60) & 42.76 & 39.87 & 42.50         & 0.028 & ~25.2 & ~913 \\
         NGC~7469 &      S1.5 & 0.0151 & ~62.7     & 43.33 (20.61) & 43.09 & 41.44 & 43.87         & 0.040 & ~73.1 & 1808 \\ 
         \hline
\end{tabular}
\tablefoot {\tablefoottext{a}{AGN types from \citet{Ver06}: S: Seyfert, L: LINER;}
\tablefoottext{b}{luminosity distance based on CMB~reference frame redshifts from NED and $H_0=73$, $\Omega_{\rm m}=0.27$, and $\Omega_{\rm vac}=0.73$;}
\tablefoottext{c}{$\Lx$~= absorption-corrected 2$-$10~keV luminosity from \citet{Dad07}, except for NGC~3227 \citep{Tue08}, logarithmic intrinsic Hydrogen column densities~$\nh$ in units of~cm$^{-2}$ from \citet{Tue08}, except ESO~\mbox{323--G77} (average of \citealt{Bec06}; \citealt{Mal07});}
\tablefoottext{d}{$\Lv\equiv\nuLnu$(5500~$\AA$); from \citet{Ben09}, except NGC~7213 \citep{Win92a}, ESO~323--G77 \citep{Sch03}, and MCG--6--30--15 \citep{Ben06}. Additional extinction correction applied to IC~4329A and ESO~323--G77 \citep{Win92b}, and NGC~3783 \citep[$A_V=1.0$ from H$\alpha$/H$\beta$;][]{Gri92};}
\tablefoottext{e}{[\ion{O}{iii}] total line fluxes from \citet{Stt03} (NGC~3783, NGC~4593, MCG--6--30--15, NGC~7213), \citet{Mel08} (NGC~3227, IC~4329A, MARK~509, NGC~7469), and \citet{Sch03} (ESO~323--G77);}
\tablefoottext{f}{$\Lm\equiv\nuLnu(12~\micron)$; this work;}
\tablefoottext{g}{from the fit to $K$-band reverberation mapping data as shown in \citet{Kis07}; observed $U-J$ or $U-K$ time lag radii: 0.071~pc (NGC~3783), 0.084~pc (MARK~509), 0.044~pc (NGC~7469);}
\tablefoottext{h}{spatial scale corresponding to the theoretical diffraction limit for a 8.2~m VLT telescope: 0$\farcs$25 at 8~$\micron$, 0$\farcs$31 at 10~$\micron$, 0$\farcs$37 at 12~$\micron$.}}
\end{table}