\begin{table}%t3
\caption{Relative line fluxes.
\label{sfluxes}}
%\centerline
 {
\begin{tabular}{llllllllll}
\hline\hline \noalign{\smallskip} & \multicolumn{3}{c}{Area BI} &
\multicolumn{3}{c}{Area BII} & \multicolumn{3}{ c}{Area E} \\ 
Line (\AA) & $F^{a}$ & $I^{b}$ & {\it S/N}$^{c}$ & $F$ & $I$ & $S/N$ & $F$ &
$I$ & S/N \\ 
\hline \hbeta\ 4861 & 9 & 35 & (27) & 11 & 35 & (11) & 13 & 35 & (25) \\ 
\oxygen\ 4959 & 6 & 20 & (20) & 11 & 31 & (12) & 7 & 18 & (17) \\
\oxygen\ 5007 & 7 & 29 & (33) & 14 & 39 & (18) & 18 & 43 & (39) \\ 
\oi\ 6300 & 4 & 5 & (35) & 6 & 7 & (14) & 6 & 7 & (33) \\ 
\nitrogen\ 6548 & 26 & 26 & (160) & 20 & 20 & (44) & 16 & 15 & (74) \\ 
\ha\ 6563 & 100 & 100 & (441) & 100 & 100 & (162) & 100 & 100 & (276) \\ 
\nitrogen\ 6583 & 81 & 79 & (373) & 63 & 62 & (109) & 47 & 47 & (163) \\ 
\sulfur\ 6716 & 30 & 27 & (161) & 28 & 26 & (52) & 19 & 18 & (81) \\ 
\sulfur\ 6731 & 24 & 21 & (129) & 22 & 20 & (41) & 14 & 13 & (62) \\
\hline Absolute \ha\ flux$^{\rm d}$ & \multicolumn{3}{c}{3} &
\multicolumn{3}{c}{2} & \multicolumn{3}{c}{7} \\
%\ha /\hbeta\  & 11.0 (27) & 8.8 (11)  & 7.29 (25)\\
\sulfur/\ha\ & \multicolumn{3}{c}{0.50 $\pm$ 0.03} &
\multicolumn{3}{c}{0.48 $\pm$ 0.07} & \multicolumn{3}{c}{0.33 $\pm$
0.02} \\ 
$F$(6716)/$F$(6731) & \multicolumn{3}{c}{1.29 $\pm$ 0.10} &
\multicolumn{3}{c}{1.32 $\pm$ 0.25} & \multicolumn{3}{c}{1.38 $\pm$
0.12} \\
\nii/\ha\ & \multicolumn{3}{c}{1.07 $\pm$ 0.02} &
\multicolumn{3}{c}{0.83 $\pm$ 0.04} & \multicolumn{3}{c}{0.63 $\pm$
0.01} \\ 
 \oxygen/\hbeta\ & \multicolumn{3}{c}{1.40 $\pm$ 0.09} &
\multicolumn{3}{c}{2.00 $\pm$ 0.30} & \multicolumn{3}{c}{1.73 $\pm$
0.12} \\ 
$c$(\hbeta) & \multicolumn{3}{c}{1.68 $\pm$ 0.05} &
\multicolumn{3}{c}{1.38 $\pm$ 0.11} & \multicolumn{3}{c}{1.17 $\pm$
0.05} \\ 
$E_{B-V}$ & \multicolumn{3}{c}{1.16 $\pm$ 0.03} &
\multicolumn{3}{c}{0.95$\pm$ 0.08} & \multicolumn{3}{c}{0.81 $\pm$ 0.03}
\\ 
\hline
\end{tabular}}
\par
\smallskip
${^a}$ Observed fluxes normalized to $F$(H$\alpha$)~=~100 and uncorrected  
for interstellar extinction.  
\par
${^b}$ Intrinsic fluxes normalized to $F$(H$\alpha$)~=~100 and corrected  
for interstellar extinction. 
\par
${^c}$ Numbers in parentheses represent the signal-to-noise ratio of the
quoted fluxes.\\ 
$^{d}$ In units of \fluxa.  
\par
Listed fluxes are a signal-to-noise weighted average of two fluxes for
areas BI and BII.\\
The emission line ratios \sulfur/\ha, $F$(6716)/$F$(6731) and
\oxygen/\hbeta\ are calculated using the values corrected for interstellar
extinction.\\
The errors of the emission line ratios, $c$(\hbeta) and $E_{B-V}$,
are calculated through standard error propagation.
\end{table}