\begin{table}%t5
\caption{\object{IC 5117} fluxes and equivalent widths.\label{ic5117table}  }  
%\begin{center}
{
\begin{tabular}{llllc}  
\hline \hline  
Wavelength &   Ion  &       log [Flux]        &      log [{\it EW}]       & Number of\\  
(\rm {\AA})&        &(erg cm$^{-2}$ s$^{-1}$)&     (\rm {\AA})     & observations\\  
\hline  
3705.00 & HeI      & $-13.661\pm0.155$ & $0.810\pm0.211$ & 2 \\   
3712.75 & HeII     & $-13.656\pm0.032$ & $0.806\pm0.122$ & 2 \\   
3726.19 & [OII]    & $-12.337\pm0.004$ & $1.768\pm0.023$ & 2 \\   
3734.37 & H$_{13}$ & $-13.340\pm0.088$ & $0.493\pm0.261$ & 2 \\   
3750.15 & H$_{12}$ & $-13.254\pm0.021$ & $1.217\pm0.179$ & 2 \\   
3770.63 & H$_{11}$ & $-13.156\pm0.053$ & $1.502\pm0.051$ & 2 \\   
3797.90 & H$_{10}$ & $-13.014\pm0.005$ & $1.651\pm0.175$ & 2 \\   
3819.70 & HeI$^{\star}$     & $-13.700\pm0.001$ & $0.846\pm0.019$ & 2 \\   
3835.38 & H$_{9}$  & $-12.836\pm0.015$ & $1.767\pm0.016$ & 2 \\   
3868.71 & [NeIII]  & $-11.503\pm0.002$ & $2.871\pm0.071$ & 4 \\   
3889.05 & H$_{8}$  & $-12.482\pm0.013$ & $1.955\pm0.098$ & 3 \\   
3967.41 & [NeIII]  & $-11.844\pm0.003$ & $2.781\pm0.100$ & 4 \\   
4068.91 & CIII     & $-12.991\pm0.002$ & $1.382\pm0.063$ & 2 \\   
4101.74 & H$\delta$& $-12.179\pm0.012$ & $2.387\pm0.134$ & 4 \\   
4340.47 & H$\gamma$& $-11.876\pm0.003$ & $2.581\pm0.112$ & 4 \\   
4363.21 & [OIII]   & $-12.191\pm0.010$ & $2.262\pm0.077$ & 4 \\   
4387.93 & HeI      & $-13.878\pm0.152$ & $0.637\pm0.111$ & 2 \\   
4471.68 & HeI      & $-12.798\pm0.001$ & $1.783\pm0.024$ & 2 \\   
4634.14 & NIII     & $-13.576\pm0.036$ & $0.695\pm0.333$ & 4 \\   
4640.64 & NIII     & $-13.215\pm0.013$ & $0.947\pm0.291$ & 4 \\   
4685.71 & HeII     & $-12.359\pm0.001$ & $2.106\pm0.075$ & 4 \\   
4713.38 & HeI$^{\star}$     & $-13.036\pm0.003$ & $1.419\pm0.082$ & 4 \\   
4724.30 & [NeIV]   & $-14.154\pm0.057$ & $0.270\pm0.163$ & 4 \\   
4740.18 & [ArIV]   & $-12.661\pm0.001$ & $1.813\pm0.029$ & 4 \\   
4861.20 & H$\beta$ & $-11.380\pm0.020$ & $3.032\pm0.006$ & 6 \\   
4921.93 & HeI      & $-13.180\pm0.050$ & $1.019\pm0.063$ & 4 \\   
4958.52 & [OIII]   & $-10.629\pm0.023$ & $3.270\pm0.124$ & 5 \\   
5007.57 & [OIII]   & $-10.131\pm0.017$ & $3.743\pm0.026$ & 2 \\   
5191.80 & [ArIII]  & $-14.152\pm0.159$ & $0.151\pm0.004$ & 4 \\   
5197.90 & [NI]     & $-13.852\pm0.019$ & $0.488\pm0.116$ & 4 \\   
5411.52 & HeII     & $-13.276\pm0.042$ & $1.107\pm0.019$ & 4 \\   
5517.72 & [ClIII]  & $-14.084\pm0.025$ & $0.209\pm0.072$ & 4 \\   
5537.89 & [ClIII]  & $-13.544\pm0.005$ & $0.801\pm0.007$ & 4 \\   
5754.59 & [NII]    & $-12.653\pm0.006$ & $1.650\pm0.005$ & 2 \\   
5875.97 & HeI      & $-11.909\pm0.024$ & $2.325\pm0.109$ & 9$\dagger$ \\   
6300.30 & [OI]     & $-12.177\pm0.026$ & $1.881\pm0.050$ & 8$\dagger$ \\   
6312.10 & [SIII]   & $-12.606\pm0.039$ & $1.437\pm0.011$ & 9$\dagger$ \\   
6363.77 & [OI]     & $-12.656\pm0.024$ & $1.453\pm0.038$ & 9$\dagger$ \\   
6548.05 & [NII]    & $-11.733\pm0.032$ & $1.612\pm0.116$ & 9$\dagger$ \\   
6562.85 & H$\alpha$& $-10.524\pm0.002$ & $2.887\pm0.223$ & 3$\dagger$ \\   
6583.45 & [NII]    & $-11.272\pm0.008$ & $2.312\pm0.184$ & 7$\dagger$ \\   
6678.15 & HeI      & $-12.366\pm0.003$ & $1.743\pm0.007$ & 9$\dagger$ \\   
6716.47 & [SII]    & $-12.958\pm0.006$ & $1.151\pm0.015$ & 9$\dagger$ \\   
6730.85 & [SII]    & $-12.612\pm0.008$ & $1.495\pm0.037$ & 9$\dagger$ \\   
7065.71 & HeI      & $-11.860\pm0.009$ & $2.200\pm0.044$ & 9$\dagger$ \\   
\hline  \\[-2mm]
\end{tabular}  }
\parbox{10cm}{
$^\star$ HeI lines are a double blend.\\
$\dagger$ Measured values were determined from two nights of observation. } 
%\end{center}
\par
\end{table}