\begin{table} %t3
\caption{Relative line fluxes.}
\label{sfluxes}
%\centerline
{
\begin{tabular}{lllllllll}
     \hline
     \hline
              & I (NE)   & II (S)  & III (NW)  & IV (CW)    & IVa (CW)& V (CE) &  Va (CE)  \\
\hline 
Line (\AA)    & $F^{\rm 1,2}$ & $F^{\rm 1,2}$ & $F^{\rm1,2}$   & $F^{\rm 1,2}$   & $F^{\rm 1,2}$ & $F^{\rm 1,2}$ & $F^{\rm 1,2}$  \\
\hline 
4861 \hbeta\   &   --     &  8 (4)  &  8 (12)   &  12 (8)   & 8 (7)    & 10 (20) & 9(8)     \\
%\hline 
5007 \oiii\    &   5 (2)  & --      & 5 (8)     &  3 (2)    & --       & 3 (7)   & 2(2)      \\
%\hline 
5200 \no\      &   --    & 5 (4)    &  --       &  2 (3)   & 10 (14)   & --      &  --      \\
%\hline 
6300 \oi\   &  14 (9)    &  12 (13) &   8 (13)  &  19 (19) & 41 (51)   & 18 (61) &  5 (7)     \\
%\hline 
6364 \oi\   &5 (3)       &  5 (5)   &   2 (4)   &   5 (5)  & 13 (18)   & 5 (15)  &  2 (1)      \\
%\hline 
6548 \nii\  &  34 (21)  &16 (18)    &  25 (44)  &  29 (29)  & 38 (43)   & 17 (54) & 19 (26)    \\
%\hline 
6563 \ha\   & 100 (58)  & 100 (94)  & 100(167)  & 100 (90)  & 100 (110) & 100 (204) & 100(129)	   \\
%\hline 
6584 \nii\  & 113 (66)  &  53 (51)  &78 (135)   &  93 (92)  & 123 (137) & 54 (159)  & 60(79)      \\
%\hline 
6716 \sii\  &   66 (46) &  47 (45)  &49 (89)    &  62 (64)  & 116 (132) & 29 (93)  & 34(48)      \\
%\hline 
6731 \sii\  &   49 (35) & 36 (35)   &37 (68)    &  47 (49)  & 87 (99)   & 22 (69)  & 25 (36)\\ 
%\hline 
\hline
Absolute \ha\ flux $^{\rm 3}$   & 31 & 60    & 66          & 50        & 62         & 48         & 67     \\
%\hline 
\ha /\hbeta\           & --      & 13 (4)    & 12 (12)    & 8.2 (8)     & 12 (7)     & 10 (20)        & 11 (8)   \\ 
%\hline 
\no /\hbeta\          & --      & 0.6 (3)    &  --       & 0.2 (3)     & 1.3 (6)     & --         & --   \\ 
%\hline 
\nii /\ha\            & 1.5 (42)& 0.7 (46)   & 1.03 (100) & 1.2 (62)   & 1.6 (83)    & 0.7 (122)  & 0.8 (65)   \\ 
%\hline 
\sii/\ha\        & 1.15 (45)    & 0.89 (49)   & 0.86 (93)  &  1.09 (60) & 2.03 (91)  & 0.51(107)  & 0.59 (54) \\ 
%\hline 
I(6716)/I(6731)& 1.35 (28)    & 1.31(28)    &  1.32 (54) &  1.32 (39)  & 1.33 (79) & 1.32 (55)& 1.36 (29) \\
%\hline 
\hline 
$c^{\rm 4}$    & --           & 1.9 [0.3]   & 1.9  [0.1]  &  1.3 [0.2]  &  1.9 [0.2]& 1.58 [0.07]  & 1.7 [0.2] \\ 
%\hline 
$E(B-V)$         & --           & 1.3 [0.2]   & 1.26 [0.07] &  0.9 [0.1]  & 1.3 [0.1] & 1.05 [0.05]   & 1.1 [0.1] \\ 
%\hline 
$n_{\rm e}$ (\dens)&  70 $\pm$ 50 & 110 $\pm$ 50  &  100 $\pm$ 20  &100 $\pm$ 30  & 90 $\pm$ 20   & 100 $\pm$ 20 
& 60$^{+50}_{-40}$    \\ 
\hline
\end{tabular}}
\smallskip
 $^1$ Uncorrected for interstellar extinction.
\par
$^2$ Listed fluxes are a signal to noise weighted
average of the individual fluxes.
\par
$^3$ In units of \flux.
\par
$^4$ The logarithmic extinction is determined as $c = 1/0.331$ $\cdot$ log((\ha/\hbeta)$_{\rm obs}$/3).
\par
 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.\\
 All fluxes are normalized to $F$(\ha) = 100.
\end{table}