\begin{table}%T1
\caption{\label{tab1}Fluxes (in units of~10$^{-15}$~erg~s$^{-1}$~cm$^{-2}$) of 
the emission lines detected in the spectrum acquired in Loiano. Values 
are corrected for Galactic absorption.}
%%\centering
\par
\begin{tabular}{lr}
\hline
\hline
\multicolumn{1}{c}{Line} & \multicolumn{1}{c}{Flux} \\
\hline
$[$O {\sc ii}$]$ $\lambda$3727  &   $ 1.51 \pm 0.15$\\
H$_\beta$                        &  $  1.1 \pm 0.2 $~~~\\
$[$O {\sc iii}$]$ $\lambda$5007 &   $ 0.35 \pm 0.09$ \\
$[$N {\sc ii}$]$ $\lambda$6548  &   $ 0.90 \pm 0.18$ \\
H$_\alpha$                       &  $  6.4 \pm 0.3 $~~ \\
$[$N {\sc ii}$]$ $\lambda$6583  &   $ 2.90 \pm 0.15$\\
$[$S {\sc ii}$]$ $\lambda$6716 &    $ 0.63 \pm 0.13$ \\
$[$S {\sc ii}$]$ $\lambda$6731 &    $ 0.86 \pm 0.17$ \\
\hline
\end{tabular}
\end{table}