\begin{table}%t1
\caption{SFRs (Cols.~2 and~3) and SFR densities (Cols.~4 and~5) of the discovered UCNR, as determined from the H$\alpha$ and UV~images. Foreground dust extinction of
$A_{{\rm H}\alpha}=A_{\rm UV}=2$~mag was assumed in all cases.}\label{table}
%%\centering
\par
\small
\begin{tabular}{l c c c c}
\hline \hline
%&&&& \\[-8pt]
Galaxy & $\rm{H}\alpha$  $(M_{\odot}~\rm{yr}^{-1})$ &  UV  $(M_{\odot}~\rm{yr}^{-1})$ & $\rm{H}\alpha$  $(M_{\odot}~\rm{yr}^{-1} \rm{pc}^{-2})$ & UV $(M_{\odot}~\rm{yr}^{-1}~\rm{pc}^{-2})$\\
\hline
%&&&& \\[-8pt]
NGC~2985 & 0.026 & 0.050 & $1.8 \times 10^{-6}$ & $3.4 \times 10^{-6}$ \\
NGC~4579 & 0.042 & 0.064 & $1.5 \times 10^{-6}$ & $2.3 \times 10^{-6}$ \\
NGC~4800 (inner UCNR) & 0.00063 & $-$  & $2.7 \times 10^{-7}$ & $-$\\
NGC~4800 (outer UCNR) & 0.030 & $-$  & $6.0 \times 10^{-7}$ & $-$ \\
\hline
\end{tabular}
\end{table}