\begin{table}
\caption{Emission line fluxes and equivalent widths in the integrated spectrum 
of the H {\sc ii} region. \label{tab4}}
\begin{tabular}{lrrrrr} \hline
Line            &
\multicolumn{1}{c}{$F$($\lambda$)$^{a}$}  &
\multicolumn{1}{c}{100$\times$$F$($\lambda$)/$F$(H$\beta$)}&
\multicolumn{1}{c}{$I$($\lambda$)$^{\rm a}$}  &
\multicolumn{1}{c}{100$\times$$I$($\lambda$)/$I$(H$\beta$)}&
$EW$($\lambda$)$^{b}$ \\ \hline
3727 [O {\sc ii}]        & $228.1\pm7.1$& $21.87\pm0.68$& $468.0\pm14.9$  & $25.82\pm0.82$& $23.95\pm0.45$ \\ 
3798 H10                 &  $49.1\pm4.4$&  $4.71\pm0.42$& $114.4\pm12.1$  &  $6.31\pm0.67$&     
                            $6.12\pm0.40$ \\ 
3835 H9                  &  $60.4\pm6.3$&  $5.79\pm0.60$& $138.1\pm16.3$  &  $7.62\pm0.90$&  
                            $6.67\pm0.62$ \\ 
3868 [Ne {\sc iii}]      & $218.9\pm10.2$  & $20.99\pm0.98$& $438.4\pm20.7$  & $24.19\pm1.14$& 
                           $24.21\pm1.10$ \\ 
3889 He {\sc i}+H8       & $175.8\pm13.4$  & $16.86\pm1.28$& $365.8\pm28.8$  & $20.18\pm1.59$&  
                           $21.73\pm1.20$ \\ 
3968 [Ne {\sc iii}]+H7   & $225.0\pm3.8$& $21.57\pm0.36$& $458.4\pm10.3$  & $25.29\pm0.57$& 
                           $26.58\pm0.20$ \\ 
4026 He {\sc i}          &  $15.3\pm1.3$&  $1.47\pm0.12$&  $29.9\pm2.4$&  $1.65\pm0.13$&  
                            $1.73\pm0.13$ \\ 
4101 H$\delta$           & $268.3\pm4.4$& $25.72\pm0.42$& $532.9\pm11.4$  & $29.40\pm0.63$& $30.79\pm0.24$ \\ 
4340 H$\gamma$           & $462.8\pm7.7$& $44.37\pm0.74$& $870.9\pm15.4$  & $48.05\pm0.85$& $79.26\pm0.57$ \\ 
4363 [O {\sc iii}]       & $102.4\pm3.7$&  $9.82\pm0.35$& $190.0\pm6.9$& $10.48\pm0.38$& $19.32\pm0.51$ \\ 
4471 He {\sc i}          &  $35.8\pm1.5$&  $3.43\pm0.14$&  $65.3\pm2.7$&  $3.60\pm0.15$&  $6.57\pm0.24$ \\ 
4686 He {\sc ii}         &  $36.9\pm1.8$&  $3.54\pm0.17$&  $65.4\pm3.3$&  $3.61\pm0.18$&  $6.70\pm0.26$ \\ 
4740 [Ar {\sc iv}]       &   $9.3\pm1.1$&  $0.89\pm0.11$&  1$6.3\pm2.0$&  $0.90\pm0.11$&  $1.76\pm0.24$ \\ 
4861 H$\beta$            &$1043.0\pm15.3$  &$100.00\pm1.47$&$1812.5\pm27.0$  &$100.00\pm1.49$&$213.40\pm0.61$ \\ 
4921 He {\sc i}          &  $12.0\pm1.6$&  $1.15\pm0.15$&  $20.5\pm2.7$&  $1.13\pm0.15$&  $2.58\pm0.41$ \\ 
4959 [O {\sc iii}]       &$1078.0\pm15.6$  &$103.36\pm1.50$&$1842.0\pm26.8$  &$101.63\pm1.48$&$204.80\pm0.27$ \\ 
5007 [O {\sc iii}]       &$3214.0\pm46.4$  &$308.15\pm4.45$&$5458.5\pm79.4$  &$301.16\pm4.38$&$576.20\pm0.34$ \\ 
5876 He {\sc i}          & $115.9\pm1.8$& $11.11\pm0.17$& $178.2\pm2.9$&  $9.83\pm0.16$& $27.80\pm0.16$ \\ 
6300 [O {\sc i}]         &   $8.6\pm0.6$&  $0.82\pm0.06$&  $12.5\pm0.9$&  $0.69\pm0.05$&  $2.36\pm0.15$ \\ 
6312 [S {\sc iii}]       &   $6.6\pm0.5$&  $0.63\pm0.05$&	$9.6\pm0.9$&  $0.53\pm0.05$&  $1.69\pm0.12$ \\ 
6563 H$\alpha$           &$3447.9\pm49.8$  &$330.58\pm4.77$&$4972.8\pm78.5 $ &$274.36\pm4.33$&$689.40\pm0.30$ \\ 
6583 [N {\sc ii}]        &  $12.4\pm0.5$&  $1.19\pm0.05$&  $17.9\pm0.7$&  $0.99\pm0.04$&  $2.48\pm0.09$ \\ 
6678 He {\sc i}          &  $31.8\pm0.7$&  $3.05\pm0.07$&  $45.5\pm1.1$&  $2.51\pm0.06$&  $7.46\pm0.15$ \\ 
6717 [S {\sc ii}]        &  $26.8\pm0.6$&  $2.57\pm0.06$&  $38.1\pm0.9$&  $2.10\pm0.05$&  $6.38\pm0.14$ \\ 
6731 [S {\sc ii}]        &  $21.8\pm0.7$&  $2.09\pm0.07$&  $30.8\pm1.1$&  $1.70\pm0.06$&  $5.22\pm0.16$ \\ 
7065 He {\sc i}          &  $49.1\pm1.0$&  $4.71\pm0.10$&  $68.0\pm1.6$&  $3.75\pm0.09$& $18.59\pm0.28$ \\ 
7136 [Ar {\sc iii}]      &  $21.1\pm0.8$&  $2.02\pm0.08$&  $29.0\pm1.3$&  $1.60\pm0.07$&  $7.62\pm0.29$ \\ 
7281 He {\sc i}          &  $ 7.6\pm0.7$&  $0.73\pm0.07$&  $10.3\pm0.9$&  $0.57\pm0.05$&  $2.81\pm0.29$ \\ \\
$C$(H$\beta$)           &\multicolumn{5}{c}{$0.240\pm0.019$} \\
{\it EW}$_{\rm abs}$$^{b}$     &\multicolumn{5}{c}{$0.9\pm0.4$} \\
\hline
\end{tabular}
\par
$^{a}$In units 10$^{-16}$ erg s$^{-1}$ cm$^{-2}$.
\par
$^{b}$In \AA.
\par
\end{table}