\begin{table} %t3
\caption{\label{tabletemplate} Template subtraction details$^a$.}
%\centering
%\small\def\footnoterule{}
\begin{tabular}{lcc}
\hline
\hline
\multicolumn{1}{c}{Galaxy} & Distance & Size\\ 
\hline
\object{IC~5063} & 23\arcsec~(NW) & 7\arcsec\\ 
\object{ESO~362-G008} & 6\arcsec~(SE) &  1\arcsec \\[0.1ex]
\object{NGC~3281} & 11\arcsec~(SW) &  \hspace*{0.2cm}1\farcs5 \\
\object{NGC~5643}$^b$ & 26\arcsec~(SW) & 2\arcsec \\
\object{NGC~1386} & 18\arcsec~(N) & 5\arcsec\\
\hline
\end{tabular}
$^a$ The template distance from the 
nucleus is given with the direction in brackets as well as the
size (diameter) of the region that was averaged to obtain the template.
The spectra were median-filtered over three pixels to increase the {\it S/N}.\\
$^b$ Template taken from VLT spectra (PA~66\degr) due to higher {\it S/N}; no reddening correction applied.
\end{table}