\begin{table}%t3
\caption{\label{tabflux}Comparison of our emission fluxes with those of \citet{Falcke98}. 
OASIS~values correspond to fluxes corrected for absorption using a combination of SSPs as
described in Sect.~3.1.  Units are  $10^{-19}~{\rm W~m}^{-2}$.}
\par
%\centering
\small
\begin{tabular}{ll|ll|ll}
\hline
\hline
Galaxy  & Aperture & \multicolumn{2}{c|}{OASIS data} &
\multicolumn{2}{c}{\citet{Falcke98}}\\
& radius   & [\ion{O}{iii}]& {H$\alpha$} + [\ion{N}{ii}] & 
[\ion{O}{iii}]& {H$\alpha$} + [\ion{N}{ii}]\\
\hline
Mrk 34  & 2\arcsec      & 4800 & 3400  & 6100 & 3600 \\
& 0.5\arcsec    & 500   &  300    & 1300  & 700 \\
\hline
Mrk 348 & 1.5\arcsec    & 3000   & 2500  & 4100  & 2000 \\
& 0.4\arcsec    & 1500   & 1000  & 3200  & 1500 \\
\hline
NGC 4388& 6\arcsec      & 9800   & ---  & 11~700    & --- \\
& 1\arcsec      & 3200   & ---  & 3900     & --- \\
\hline
\end{tabular}
\end{table}