\begin{table}%t2
        \caption{Relative line fluxes.}
         \label{sfluxes}
%\centerline
{ \begin{tabular}{lllllll}
\hline     \hline
           &Area Ia       & Area Ib  & Area IIa   & Area IIb     &Area IIc &Area IId \\
\hline\noalign{\smallskip}
Line (\AA) & $F^{a,b}$ & $F^{a,b}$  & $F^{a,b}$ &$F^{a,b}$&$F^{a,b}$    \\
\hline
4861 \hbeta\    & 9.8 (6)& 14.4 (6)  &17.9 (19)&15.8 (28)&13.4 (23)& 18.5 (25)  \\
\hline
4959 \oiii$_1$ & --      & --        &2.6 (3)  &2.1 (4)  &0.9 (2)  & 1.8 (2)   \\
\hline
5007 \oiii$_2$ & 4.9(3)  & 8 (3)     &10.2 (12)&7.0 (13) &3.8 (7)  & 6.4 (10) \\
\hline  
5876 He I     & --      & --        & 2.8 (6) &2.7 (11) &2.3 (8) & 2.0 (7)  \\ 
\hline  
6300 \oi$_1$  & 3.8 (2)  & --        &2.1 (5)  &0.9 (5)  &0.7 (3) & 2.7 (12) \\
\hline
6364 \oi$_2$  &  --      &  --       & --      &--       &    --  & 0.7 (3) \\
\hline
6548 \nii$_1$ & 9.4 (12)  & 5.0 (3)  &12.2 (27)&11.9 (52)&11.7 (47)&12.7 (44)      \\
\hline
6563 \ha\     & 100 (122) & 100 (68) &100 (207)&100 (376)&100 (354)& 100 (293)      \\
\hline
6584 \nii$_2$ & 53.7 (66) & 39.4 (27)&44.6 (97)&39.7 (168)&43.3 (165)& 45.7 (135)      \\
\hline
6716 \sii$_1$ & 29.6 (42) & 13.2 (10)&13.4 (32)&11.5 (52)&13.8 (58)  & 16.5 (57)     \\
\hline
6731 \sii$_2$ & 31.2 (44) & 11.2 (9) &12.2 (29)&11.9 (54)&13.9 (58)  & 16.7 (57)   \\
\hline 
\hline
Absolute \ha\ flux$^{c}$ & 56   & 50      & 81        & 149      &239    & 62\\
\hline
\ha /\hbeta\             & 10.2 (6)  &  6.9 (6) & 5.6 (19)  &6.3 (28)  & 7.5 (23) & 5.4 (25) \\
\hline
$c$                     & 1.6 [0.2] & 1.1 [0.2] & 0.82 [0.07]&0.97 [0.05]& 1.20 [0.06]&0.77 [0.05] \\
\hline
\oiii /\hbeta            & 0.7 (3)   & --        & 0.76 (10) & 0.59 (12)& 0.38 (7) &0.46 (9)\\ 
\hline
\sii/\ha\                & 0.61 (54) & 0.24 (13)& 0.26 (43) & 0.23 (74)& 0.28 (80)&0.33 (81) \\
\hline 
$I$(6716)/$I$(6731)        & 0.95 (30) & 1.1 (7)  & 1.09 (21) & 0.97 (37)& 0.99 (41)& 0.99 (40)\\
\hline 
\end{tabular}}
 ${^a}$ Fluxes uncorrected for interstellar extinction and relative to
 $F({\rm H}\alpha)=100$.\\
${^b}$ Listed fluxes are a signal to noise weighted
average of the individual fluxes.\\
$^{c}$ In units of \flux. \\
 Numbers in parentheses represent the signal to noise ratio 
of the quoted fluxes.  The 1$\sigma$ error is given in square brackets for the logarithmic 
extinction.
\end{table}