\begin{table}%t2
%\centering
\par
\caption{Fluxes for the strong emission lines in units of 
10$^{-16}$~erg~s$^{-1}$~cm$^{-2}$ corrected for Galactic extinction. The
  magnitudes are given in AB units. The first three rows correspond
    to different aperture sizes.  For the WR and SN region the
  radial apertures are~2\arcsec\ defined to include all the flux from
  the regions seen in the \halpha~image.  Below the first three rows
    the fluxes are extracted from the images in a square
  aperture of $3\times3$~spaxels equivalent to 4~arcsec$^2$ around the
  coordinates in Col.~1.  The magnitudes are calculated from
    the spectra extracted within this aperture. Note that the
  properties vary with the chosen aperture; especially the equivalent
  widths show differences as described in Sect.~\ref{sect:ew}.
    The oxygen abundance and N/O~abundance ratio in the two
  last columns are discussed in Sect.~\ref{sect:metal}. The
  uncertainties for line fluxes and magnitudes are $\approx$10\%,
  $<$4\%   for the \halpha\ and \hbeta\ {\it EW}, 0.12~mag for the
  reddening, and 0.14~dex for the oxygen abundance calibration. The
  uncertainty of the N/O~ratio is 0.2~dex. The last row gives the
     mean of the individual regions, and the uncertainty is
  the standard deviation.
\label{tab:emlines}}
$$
\begin{tabular}{l@{} r@{.}l @{}r@{.}l  @{}r@{.}l  @{}r@{.}l  r@{.}l  r@{.}l
    r@{.}l  r@{.}l @{}r@{.}l @{}cccc @{}c @{}c@{}}
\hline
\hline
\noalign{\smallskip}
Region & \multicolumn{2}{c}{[\ion{O}{ii}]} &
\multicolumn{2}{c}{\hbeta} & \multicolumn{2}{c}{[\ion{O}{iii}]} &
\multicolumn{2}{c}{\halpha} & \multicolumn{2}{c}{[\ion{N}{ii}]} &
\multicolumn{2}{c}{[\ion{S}{ii}]} & \multicolumn{2}{c}{[\ion{S}{ii}]}
& \multicolumn{2}{c}{{\it EW}(\halpha)} & \multicolumn{2}{c}{{\it EW}(\hbeta)} 
& $B$ & $V$ & $R$  & \ebv &
12~+~log(O/H) & log(N/O) \\
 &   \multicolumn{2}{c}{$\lambda$3727} & \multicolumn{2}{c}{} &
\multicolumn{2}{c}{$\lambda$5007} & \multicolumn{2}{c}{}  &
\multicolumn{2}{c}{$\lambda$6584} & \multicolumn{2}{c}{$\lambda$6716}
& \multicolumn{2}{c}{$\lambda$6731} & \multicolumn{2}{c}{$({\AA})$} & 
\multicolumn{2}{c}{$({\AA})$} &  (mag)  & (mag) & (mag) & (mag) \\
%(1) & \multicolumn{2}{c}{(2)} & \multicolumn{2}{c}{(3)} & \multicolumn{2}{c}{(4)} & \multicolumn{2}{c}{(5)} & \multicolumn{2}{c}{(6)} & \multicolumn{2}{c}{(7)} & \multicolumn{2}{c}{(8)} & (9) & (10) & (11) &(12) & (13) \\  
\noalign{\smallskip}
\hline
\noalign{\smallskip}
Galaxy & 2400&0 & 445&0 & 1293&0 & 1793&0  & 197&0 & 283&0   & 68&0 &
67& & 13& &  15.31 & 15.08  & 14.85 & 0.30 & 8.27 & --1.50 \\
WR reg & 694&6 & 174&0 & 815&0 & 603&0 & 47&9 & 51&9 & 39&78 &744& &
141& & 18.64 & 
18.27  & 18.3 & 0.17 & 8.16 & --1.50 \\
SN reg & 26&07 & 7&55 & 18&27 & 44&94 & 5&03 & 9&19 & 6&84 & 178& & 
16& & 20.28 & 
20.21 & 19.8 & 0.63 & 8.30  & --1.28 \\
\hline
\noalign{\smallskip}
\par
WR(--8.7, 0.0) & 436&5 & 142&0 & 719&0 & 419&0 & 30&2 & 30&5 & 24&1 &
1140& & 226& & 
19.16 & 18.72 & 18.92 & 0.03  & 8.14 & --1.42 \\ %r27
\par
SN(--5.3, --2.7)& 8&11 & 2&83 & 7&14 & 19&42 & 2&33 & 4&34 & 3&17 &
208& & 22& & 
21.28 & 21.24 & 21.17 & 0.75 & 8.31  & --1.17 \\ %r26
\par
--11.4, 11.3    & 0&80 & 0&74 & 0&57 & 9&41& 1&13 & 1&51 & 1&13 & 79&
& 6&2 & 
20.96 & 21.12 & 20.74 & 1.29 & 8.47  & --0.64   \\ %r20(41,39)
\par
--8.0, 12.0     & 2&77 & 1&47 & 1&20 & 9&23 & 1&59  & 2&43  & 1&90 &
75& & 12& & 
21.93 & 21.20 & 20.72 & 0.68 & 8.51  & --0.83 \\ %r18(35,39)
\par
--6.7, 8.0      & 1&68 & 1&11 & 1&40 & 7&75 & 0&96 & 1&36 & 1&15 & 38&
&  5&2 & 
21.04 & 20.57 & 20.24 & 0.78 & 8.41  & --0.88 \\ %r24(33,33)
\par
--4.0, 7.3      & 6&30 & 3&43 & 3&89 & 16&08 & 2&01 & 2&50 & 1&83 &
62& & 12& & 
20.59 & 20.22 & 19.92 & 0.43 & 8.41  & --0.98 \\ %r14(29,32)
\par
--2.0, 14.0     & 6&43 & 2&01 & 2&60 & 11&13 & 1&57 & 1&89 & 1&54 &
74& & 12& & 
21.28 & 20.80 & 20.50 & 0.57 & 8.42  & --1.16 \\%r16(26,42)
\par
--1.3, --6.1    & 3&80 & 1&70 & 2&37 & 17&68 & 2&05 & 3&13 & 2&19 &
420& &  16& & 
21.47& 21.52 & 21.37  & 1.12 & 8.38  & --1.00 \\ %r2(25,12)
\par
--1.3, 10.0     & 2&13 & 1&45 & 0&92 & 7&87 & 1&15 & 1&53 & 1&25 & 34&
&  5&6 &
20.67& 20.35 & 20.06 & 0.56 & 8.53   & --0.81 \\ %r21(26,37)
\par
--0.7, 1.3      & 34&1 & 11&80 & 25&51 & 48&51 & 6&29 & 5&04 & 3&61 &
119& &  25& & 
20.14 & 19.65 & 19.38 & 0.32 & 8.34  & --1.15 \\ %r13(24,32)
\par
--0.0, 3.3      & 2&19 & 1&32 & 3&13 & 7&56 & 1&22 & 1&62 & 1&22 & 29&
&  4&5 &
20.65 & 20.21 & 19.94 & 0.60 & 8.36  & --0.84 \\%r22(24,27)
\par
2.0, 12.7       & 0&00 & 0&84 & 0&83 & 5&25 & 0&73 & 1&27 & 1&08  &
230& & 4&9 & 
21.17 & 20.76 & 20.43 & 0.67 & 8.46  & ... \\ %%r17(21,41)
\par
2.7, 1.3        & 4&34 & 4&20 & 3&52 & 17&25 & 2&56 & 2&77 & 1&83 &
296& & 15& & 
20.44 & 20.44 & 20.26 & 0.32 & 8.49  & --0.65 \\ %r12(19,23)
\par
2.7, --4.0      & 6&34 & 0&92& 1&27  & 10&97 & 1&59 & 2&76 & 1&96 &
2411& &  13& & 
21.73 & 21.87 & 21.82 & 1.23 & 8.42  & --1.32 \\ %r3(19,11)&  
\par
5.4, 6.0        & 2&84 & 3&04 & 2&76 & 13&14 & 1&91 & 2&34 & 1&72 &
38& &  7&3 & 
20.23 & 19.86 & 19.62 & 0.36 & 8.48  & --0.62 \\ %r10(15,30)
\par
6.1, 10.7       & 5&59 & 4&57& 4&74  & 16&04 & 2&44 & 3&50 & 2&48 &
58& & 12& & 
 20.25 & 19.98 & 19.85 & 0.18 & 8.46 & --0.70 \\ %r11(14,37)
\par
8.7, 0.6        & 8&15 & 6&65 & 3&40 & 15&95 & 2&04 & 4&53  & 2&84 &
49& &   17& & 
20.16 & 19.90 & 19.37 & 0.00 & 8.54  & --0.83 \\ %r6(10,22)
\par
9.4, --3.3      & 28&3 & 17&39 & 37&42 & 42&96 & 4&77 & 7&03 & 5&20 &
254& &  56& & 
21.24 & 21.02 & 21.07 & 0.00 & 8.32  & --1.00 \\ %r5(9,12) 
\par
10.1, 8.0       & 0&24 & 2&70 & 4&96 & 10&82 & 1&33 & 1&83  & 1&31 &
47& &  8&2 & 
20.26 &  20.18 &  20.19 & 0.29 & 8.35& --0.64 \\%r9(8,33) 
\par
11.4, 4.6       & 21&7 & 12&18 & 27&19 & 27&10 & 4&52 & 4&07& 3&02 &
149& &  19& &
19.63 & 19.43 &  18.94  & 0.00 & 8.37& --0.92 \\ %r8(6,28) 
\par
12.1, 13.3      & 0&00 & 0&77& 0&76 & 3&68 & 0&52 & 0&70 & 0&59 & 38&
&  4&7 & 
21.27 & 20.97 & 20.99  & 0.45 & 8.46 & ...\\  %%r19(6,42) 
\par
14.8, 3.3       & 13&6 & 3&42& 6&00 & 9&25 & 1&00 & 1&92 & 1&34 & 61&
& 15& & 
20.70 & 20.55 & 20.08 & 0.00 &  8.34 & --1.36\\ %r7(1,26) 
\par
14.8, 10.0      & 7&49 & 3&48 & 4&85 & 7&28 & 1&16 & 1&53 & 1&39 & 79&
& 25& & 
21.11 & 21.08 & 20.98 & 0.00 & 8.43  & --1.03\\ %r15(1,36)
\par
\hline
Mean     &29&~$\pm$~94 & 10&~$\pm$~29 & 38&~$\pm$~149 & 33&~$\pm$~85 &3&~$\pm$~6
&4&~$\pm$~6 &3&~$\pm$~5 & 152&~$\pm$~243 &   24&~$\pm$~46 & 20.5~$\pm$~0.6 & 20.3~$\pm$~0.7&
20.0~$\pm$~0.6 & 0.46~$\pm$~0.40  & 8.41~$\pm$~0.09 & --0.91~$\pm$~0.34\\
\hline
\end{tabular}
$$
\end{table}