\begin{table}%t3
        \caption{\label{sfluxes}Relative line fluxes.}
         \small%\centerline
{
               \begin{tabular}{lllllllll}
     \hline\hline
            & I            & II     & III     & IV      & V       & VI   &  VII  \\
\hline\noalign{\smallskip}
Line (\AA) & F            & F       & F        & F      & F        & F       & F      \\
%\hline
4861 \hbeta\   & --        & 9 (3)   &  15 (4)  &  --   &  20 (8)    &18 (5)  & --  \\
%\hline
6300 \oi      & 17 (6)     & 17 (9)  & 9 (3)    & --    &  --       &--      &30 (6) \\
%\hline 
6548 \nii     & 20 (7)     & 15 (6)  & 15 (6)   & 14 (5) &  14 (7)  &13 (6)  &16 (3)   \\
%\hline
6563 \ha\     & 100 (33)   & 100 (46)& 100 (37) & 100 (33)& 100 (49)&100 (43)&100 (19)    \\
%\hline
6584 \nii    & 65 (21)    & 44 (20) & 44 (16)  & 50 (17) & 46 (23)  &53 (22) &52 (10)   \\
%\hline
6716 \sii    & 59 (20)    & 48 (23) & 38 (15)  & 27 (9)  & 26 (13)  &31 (12) &45 (9)     \\
%\hline
6731 \sii   & 48 (17)    & 34 (16) & 26 (11)  & 20(7)  & 20 (10)    &22 (9)  &34 (7)  \\
\hline \noalign{\smallskip}
%\hline
Absolute \ha\ flux$^{\rm 1}$ & 6.5 &  12.8  & 15.5& 10.5 & 13.5      &6.5     &5.7 \\
\hline
\ha /\hbeta\     & --        & 11 (3) &   7 (4)    & --  & 5.0 (8)      &5.5 (5) &--   \\
%\hline
\sii/\ha\        & 1.08 (20) & 0.83 (24) &0.64 (16)&0.47 (11)& 0.46 (16)&0.53 (14)& 0.80 (10) \\
%\hline 
I(6716)/I(6731)& 1.23 (13) & 1.41 (13) &1.45 (9)&1.37 (6)& 1.30 (8)  & 1.36 (7) &1.31 (6)  \\
%\hline 
n$_{\rm e}$$^{\rm 2}$    & $<$380 \dens & $<$120 \dens & $<$130 \dens & $<$320 \dens & $<$330
\dens & $<$290 \dens & $<$410 \dens  \\
\hline
\end{tabular}}
\smallskip
$^{\rm 1}$ In units of \flux.\\
$^{\rm 2}$ 1$\sigma$ upper limits. \\ 
All fluxes are not corrected for interstellar extinction 
Numbers in parentheses represent the signal-to-noise ratio 
of the quoted values
All fluxes normalized to F(\ha$)=100$.
\end{table}