\begin{table}%t2
\par
\caption{Observed and predicted line fluxes of \src.
\label{table2}}
%%\centerline

 {\begin{tabular}{c c c c c}
\hline\hline
\rule[-1.5mm]{0pt}{4ex}Line& Observed flux$^a$& Predicted flux$^b$ & Corrected flux & $A_\lambda^c$ \\
\rule[-1.5mm]{0pt}{3ex} & [\cgs] & [\cgs] &  [\cgs] & [mag] \\
\hline
\rule[-1.7mm]{0pt}{4ex} H$\alpha$    & $(5\pm0.2)\times10^{-16}$ & $1.7\times10^{-14}$ & $4.6\times10^{-15}$ & 2.4\\
\rule[-1.7mm]{0pt}{4ex} H$\beta$     & $<$$1\times10^{-16}$        & $4.8\times10^{-15}$ &      $-$            & 5.3\\
\rule[-1.7mm]{0pt}{4ex} [O{\sc iii}] & $<$$3\times10^{-17}$        & $2.9\times10^{-15}$ &      $-$            & $-$\\
\hline
\end{tabular}}
\par
\smallskip
$^a$ Uncorrected for extinction, measured from the IR spectrum.\\
$^b$ From the correlations of \citet{panessa2006}.\\
$^c$ Extinction estimated from the model.
\end{table}