\begin{table}%t4 
\caption []{\object{DdDm 1} fluxes and equivalent widths.\label{dddm1table}}  
%\begin{center}
{ 
\begin{tabular}{lcccc}   
\hline \hline  
Wavelength &   Ion  &       log [Flux]        &      log [{\it EW}]      & Number of   
\\  
(\rm {\AA})&	    &(erg cm$^{-2}$ s$^{-1}$)&     (\rm {\AA})    & observations   
\\  
\hline  
3726.19 & [OII]    & $-11.759\pm0.001$  & $2.184\pm0.082$ & 2 \\  
3750.15 & H$_{12}$ & $-13.321\pm0.055$  & $0.719\pm0.045$ & 2 \\   
3770.63 & H$_{11}$ & $-13.257\pm0.043$  & $0.805\pm0.040$ & 3 \\   
3797.90 & H$_{10}$ & $-13.119\pm0.035$  & $0.938\pm0.052$ & 2 \\   
3819.7  & HeI$^{\star}$     & $-13.735\pm0.120$  & $0.267\pm0.102$ & 3 \\   
3835.38 & H$_{9}$  & $-12.969\pm0.031$  & $1.077\pm0.024$ & 4 \\   
3868.71 & [NeIII]  & $-12.313\pm0.009$  & $1.752\pm0.030$ & 3 \\   
3889.05 & H$_{8}$  & $-12.511\pm0.003$  & $1.562\pm0.068$ & 3 \\   
3967.41 & [NeIII]  & $-12.382\pm0.006$  & $1.724\pm0.015$ & 2 \\   
4026.1  & HeI$^{\star}$     & $-13.466\pm0.011$  & $0.672\pm0.033$ & 2 \\   
4068.91 & CIII     & $-13.530\pm0.024$  & $0.611\pm0.023$ & 4 \\   
4101.74 & H$\delta$& $-12.400\pm0.017$  & $1.742\pm0.041$ & 4 \\   
4340.47 & H$\gamma$& $-12.124\pm0.010$  & $2.096\pm0.034$ & 3 \\   
4363.21 & [OIII]   & $-13.096\pm0.012$  & $1.126\pm0.121$ & 2 \\   
4387.93 & HeI      & $-14.101\pm0.163$  & $0.135\pm0.253$ & 3 \\   
4471.68 & HeI      & $-13.098\pm0.021$  & $1.158\pm0.066$ & 3 \\   
4861.20 & H$\beta$ & $-11.794\pm0.001$  & $2.542\pm0.032$ & 3 \\   
4959.52 & [OIII]   & $-11.623\pm0.004$  & $2.699\pm0.036$ & 2 \\   
5007.57 & [OIII]   & $-11.145\pm0.0001$ & $3.034\pm0.120$ & 2 \\   
5197.90 & [NI]     & $-14.144\pm0.002$  & $0.298\pm0.011$ & 2 \\   
5269.20 & [KVI]    & $-13.714\pm0.019$  & $0.767\pm0.002$ & 2 \\   
5517.72 & [ClIII]  & $-14.459\pm0.132$  & $0.065\pm0.096$ & 2 \\   
5537.89 & [ClIII]  & $-14.339\pm0.158$  & $0.173\pm0.155$ & 2 \\   
5754.59 & [NII]    & $-13.683\pm0.025$  & $0.906\pm0.040$ & 2 \\  
\hline  
\end{tabular} } 
\parbox{10cm}{
$^\star$ HeI lines are a double blend.}  
%\end{center}
\par
\end{table}