\begin{table}%t3
%\centering
\par
\caption{Table of emission lines used in this paper. Fluxes and {\it EW}s are as observed. Fluxes from the FORS spectrum are taken 
from Pian et~al.~(\cite{Pian06}).
\label{linestable} }
\begin{tabular}{lcc}
\hline\hline
\multicolumn{3}{c}{UVES spectrum} \\
\hline 
ID & {\it EW} & Flux \\ 
 & ({\AA})   &  ($\times 10^{-17}$ erg s$^{-1}$ cm$^{-2}$)  \\ 
\hline 
$[\ion{O}{ii}]$ $\lambda$3727 & 1.59 $\pm$  0.09 & 75.23 $\pm$ 3.42  \\
$[\ion{O}{ii}]$ $\lambda$3729 & 2.62 $\pm$  0.12  & 121.1 $\pm$ 4.0   \\
$[\ion{Ne}{iii}]$ $\lambda$3869 & 0.75 $\pm$ 0.08  & 34.06 $\pm$ 3.51   \\
$[\ion{Ne}{iii}]$ $\lambda$3969 & 0.26$\pm$ 0.06  & 11.80 $\pm$ 2.64   \\
H$\beta$ $\lambda$4862 & 2.17 $\pm$ 0.06  & 92.92 $\pm$ 1.93	 \\
H$\gamma$ $\lambda$4341 & 0.90 $\pm$ 0.07  &  47.99 $\pm$ 3.46   \\
H$\delta$ $\lambda$4102 & 0.61 $\pm$ 0.07  &  27.83 $\pm$ 3.04    \\
H$\epsilon$ $\lambda$3971 & 0.29 $\pm$ 0.07  & 13.03 $\pm$ 3.02    \\
H8 $\lambda$3889 & 0.27 $\pm$ 0.07  & 12.25 $\pm$  2.90    \\
H9 $\lambda$3835 & 0.18 $\pm$ 0.07  & 7.65 $\pm$ 2.92    \\
$[\ion{O}{iii}]$ $\lambda$4960 & 2.88 $\pm$ 0.06  &  139.0 $\pm$ 2.08  \\
$[\ion{O}{iii}]$ $\lambda$5008 & 8.34 $\pm$ 0.09  &  426.2 $\pm$ 2.48    \\
$\ion{He}{i}$ $\lambda$5877 & 0.24 $\pm$ 0.04 & 9.55 $\pm$  1.17    \\
\hline
\multicolumn{3}{c}{FORS spectrum} \\
\hline 
 ID &  & Flux \\ 
 &    &  ($\times 10^{-17}$ erg s$^{-1}$ cm$^{-2}$)  \\ 
\hline 
$[\ion{O}{ii}]$ $\lambda$3727, 3729  & & 190 $\pm$ 50 \\
(Doublet unresolved)&&\\
$[\ion{Ne}{iii}]$ $\lambda$3869&& 31 $\pm$ 5\\
$[\ion{Ne}{iii}]$ $\lambda$3969&& 18 $\pm$ 3\\
H$\gamma$ $\lambda$4341 && 37 $\pm$ 6  \\
$[\ion{O}{iii}]$ $\lambda$4364 && 21 $\pm$ 4\\
H$\beta$ $\lambda$4862&&101 $\pm$ 4\\
$[\ion{O}{iii}]$ $\lambda$4960 &&150 $\pm$ 7\\
$[\ion{O}{iii}]$ $\lambda$5008 &&460 $\pm$ 10\\
$\ion{He}{i}$ $\lambda$5877 && 5.5 $\pm$ 1.0\\
H$\alpha$ $\lambda$6563 &&315 $\pm$ 25\\
$[\ion{N}{ii}]$ $\lambda$6584 &&19 $\pm$ 2\\
$[\ion{S}{ii}]$ $\lambda$6717 &&14 $\pm$ 2\\
$[\ion{S}{ii}]$ $\lambda$6731 &&14 $\pm$ 2\\
\hline
\end{tabular} 
\end{table}