\begin{table}%T3
%\centering
\par
\caption{\label{1386linespectrum}NGC~1386: emission lines included in the fit of the soft \mbox{X-ray}\protect spectrum, along with their most likely identifications (see text for\protect details).}
\begin{tabular}{ccc}
\hline\hline
{Energy} & {Flux} & {Id.} \\
(keV) & ($10^{-5}$ ph cm$^{-2}$ s$^{-1}$) &  \\
\hline
 %&  &  \\
$\rm 0.53^{+0.01}_{-0.05}$ & $\rm 4.6^{+0.8}_{-1.5}$ & {N~\textsc{vii}} K$\alpha$--{O~\textsc{vii}} K$\alpha$ \\
% &  &  \\
$0.66\pm0.02$ & $1.3\pm0.4$ & {O~\textsc{viii}} K$\alpha$--{O~\textsc{vii}} K$\beta$\\
% &  &  \\
$0.76\pm0.01$ & $1.5\pm0.4$ & {O~\textsc{vii}} RRC--{O~\textsc{viii}} K$\beta$ \\
% &  &  \\
$\rm 0.84^{+0.02}_{-0.01}$ & $1.5\pm0.3$ & {O~\textsc{viii}} RRC \\
% &  &  \\
$\rm 0.94^{+0.01}_{-0.02}$ & $1.1\pm0.3$ & {Ne~\textsc{ix}} K$\alpha$\\
% &  &  \\
$1.05^\pm0.02$ & $0.6\pm0.2$ & {Ne~\textsc{x}} K$\alpha$ \\
% &  &  \\
$\rm 1.16^{+0.02}_{-0.01}$ & $0.5\pm0.2$ & {Fe~\textsc{xxiv}} L \\
 %&  &  \\
$1.38\pm0.04$ & $0.2\pm0.1$ & {Mg~\textsc{xi}} K$\alpha$\\
 %&  &  \\
$1.78\pm0.05$ & $0.2\pm0.1$ & {Si~\textsc{xiii}} K$\alpha$\\
% &  &  \\
\hline
\end{tabular}
\end{table}