\begin{table}%T2
\caption{\label{fluxes}Fluxes and iron line properties for the \textit{Chandra} observations analysed in this paper. The iron line fluxes and {\it EW}s refer to the "local'' fits (see text for details).}
%\centerline
{
\begin{tabular}{ccccc}
\hline\hline
{Source} & ${F}_{\rm 0.5{-}2~keV}$ $^a$ & ${F}_{\rm 2{-}10~keV}$ $^a$ & ${\it EW}_{\rm Fe}$ $^b$ & ${I}_{\rm Fe}$ $^{c}$\\
\hline
%&&&&\\
NGC~1386 & $\rm 1.8^{+1.5}_{-0.5}$ & $2.4\pm1.0$ & $\rm 1.5^{+0.8}_{-0.5}$ & $\rm 0.6^{+0.3}_{-0.2}$\\
% &  & & &\\
NGC~3393 & $\rm 2.2^{+0.5}_{-0.2}$ & $2.6\pm0.8$ & $0.6\pm0.3$ & $0.4\pm0.2$\\
% &  &  &  &\\
NGC~5347 & $\rm 0.27\pm0.06$ & $2.4\pm0.7$ & $1.7\pm0.7$ & $0.5\pm0.2$\\
% &  &  &  &\\
NGC~5643 & $1.4\pm0.2$ & $6.3^{+2.1}_{-2.0}$ & $\rm 1.5^{+0.8}_{-0.6}$ & $\rm 1.3^{+0.7}_{-0.5}$\\
% &  &  &  & \\
NGC~7212 & $\rm 0.8^{+0.1}_{-0.2}$ & $\rm 5.2^{+1.3}_{-1.2}$ & $0.7\pm0.3$ & $0.7\pm0.3$\\
 %&  &  &  &\\
 \hline
\end{tabular}}
\medskip
$^a$ In units of $10^{-13}$ erg cm$^{-2}$ s$^{-1}$; 
$^b$ Iron line {\it EW} in units of keV; 
$^c$ Iron line flux in units of $10^{-5}$ ph cm$^{-2}$ s$^{-1}$.
\end{table}