\begin{table} %t8
\caption{\object{NGC~6833} fluxes and equivalent widths.\label{ngc6833table}  }  
%\begin{center}
{
\begin{tabular}{lcccc}   
\hline \hline  
Wavelength &   Ion  &       log [Flux]        &      log [{\it EW}]      & Number of\\  
(\rm {\AA})&        &(ergs cm$^{-2}$ s$^{-1}$)&     (\rm {\AA})    & Observations\\  
\hline  
3697.15 & H$_{17}$ & $-13.829\pm0.241$ & $-0.0003\pm0.109$& 4$\dagger$ \\   
3705.00 & HeI      & $-13.288\pm0.081$ & $0.423\pm0.037$  & 4$\dagger$ \\   
3712.75 & HeII     & $-13.346\pm0.149$ & $0.401\pm0.043$  & 4$\dagger$ \\   
3726.19 & [OII]    & $-12.259\pm0.066$ & $1.358\pm0.012$  & 4$\dagger$ \\   
3734.37 & H$_{13}$ & $-12.977\pm0.116$ & $0.562\pm0.024$  & 4$\dagger$ \\   
3750.15 & H$_{12}$ & $-12.920\pm0.023$ & $0.959\pm0.004$  & 6$\dagger$ \\   
3770.63 & H$_{11}$ & $-12.812\pm0.024$ & $1.066\pm0.005$  & 6$\dagger$ \\   
3797.90 & H$_{10}$ & $-12.689\pm0.055$ & $1.184\pm0.003$  & 6$\dagger$ \\   
3819.70 & HeI$^{\star}$     & $-13.305\pm0.146$ & $0.573\pm0.076$  & 5$\dagger$ \\   
3835.38 & H$_{9}$  & $-12.540\pm0.030$ & $1.334\pm0.006$  & 6$\dagger$ \\   
3868.71 & [NeIII]  & $-11.439\pm0.020$ & $2.394\pm0.033$  & 8$\dagger$ \\   
3889.05 & H$_{8}$  & $-12.142\pm0.019$ & $1.692\pm0.024$  & 7$\dagger$\\   
3967.41 & [NeIII]  & $-11.761\pm0.001$ & $2.136\pm0.005$  & 8$\dagger$ \\   
4026.10 & HeI$^{\star}$     & $-13.025\pm0.013$ & $0.905\pm0.014$  & 5$\dagger$ \\   
4068.91 & CIII     & $-13.442\pm0.128$ & $0.481\pm0.117$  & 4$\dagger$ \\   
4101.74 & H$\delta$& $-11.954\pm0.006$ & $1.988\pm0.001$  & 7$\dagger$ \\   
4340.47 & H$\gamma$& $-11.673\pm0.037$ & $2.269\pm0.026$  & 8$\dagger$ \\   
4363.21 & [OIII]   & $-12.247\pm0.040$ & $1.715\pm0.056$  & 8$\dagger$ \\   
4387.93 & HeI      & $-13.601\pm0.042$ & $0.378\pm0.006$  & 5$\dagger$ \\   
4471.68 & HeI      & $-12.613\pm0.039$ & $1.369\pm0.030$  & 7$\dagger$ \\   
4713.38 & HeI      & $-13.244\pm0.009$ & $0.821\pm0.012$  & 6$\dagger$ \\   
4740.18 & [ArIV]   & $-13.447\pm0.034$ & $0.590\pm0.039$  & 5$\dagger$ \\   
4861.20 & H$\beta$ & $-11.315\pm0.012$ & $2.733\pm0.033$  & 7$\dagger$ \\   
4921.93 & HeI      & $-13.246\pm0.034$ & $0.785\pm0.050$  & 4$\dagger$ \\   
4959.52 & [OIII]   & $-10.886\pm0.007$ & $3.003\pm0.023$  & 4$\dagger$ \\   
5007.57 & [OIII]   & $-10.401\pm0.001$ & $3.439\pm0.074$  & 2$\dagger$ \\   
5191.80 & [ArIII]  & $-14.275\pm0.177$ & $-0.150\pm0.186$ & 2 \\   
5537.89 & [ClIII]  & $-13.935\pm0.082$ & $0.243\pm0.098$  & 2 \\   
5754.59 & [NII]    & $-13.049\pm0.047$ & $1.121\pm0.017$  & 6 \\   
5875.97 & HeI      & $-12.038\pm0.002$ & $2.112\pm0.011$  & 3 \\   
6300.30 & [OI]     & $-12.841\pm0.268$ & $1.342\pm0.272$  & 3 \\   
6363.77 & [OI]     & $-13.245\pm0.006$ & $0.966\pm0.080$  & 3 \\   
6548.05 & [NII]    & $-12.262\pm0.007$ & $1.247\pm0.038$  & 4 \\   
6562.85 & H$\alpha$& $-10.752\pm0.001$ & $2.838\pm0.051$  & 1$\ddagger$ \\   
6583.45 & [NII]    & $-11.865\pm0.003$ & $1.867\pm0.021$  & 4 \\   
6678.15 & HeI      & $-12.620\pm0.007$ & $1.598\pm0.028$  & 4 \\   
6716.47 & [SII]    & $-13.888\pm0.033$ & $0.329\pm0.035$  & 3 \\   
6730.85 & [SII]    & $-13.531\pm0.029$ & $0.700\pm0.001$ & 3 \\   
7065.71 & HeI      & $-12.130\pm0.003$ & $2.123\pm0.009$  & 3 \\   
\hline  
\end{tabular}  }
\parbox{10.5cm}{
$^\star$ HeI lines are a double blend.\\  
$\dagger$ Measured values were determined from two nights of observation. \\  
$\ddagger$ Errors are based on one measurement.  }
%\end{center}
\par
\end{table}