\begin{table}%T1
\caption{\label{fluxes}Observed line fluxes, $F_{\lambda}$, and 
intensities, $I_{\lambda}$, of nebular and stellar (Wolf-Rayet, WR) lines 
in each of the four VLT/FORS2 IC~4662 apertures, relative to H$\beta=100$. 
H$\beta$ fluxes are shown separate from normalised values in units of 
10$^{-13}$ erg s$^{-1}$ cm$^{-2}$. } 
%\centerline
 {
\begin{tabular}{
l@{\hspace{1.5mm}}c@{\hspace{1.5mm}}c@{\hspace{3mm}}
r@{\hspace{1.5mm}}r@{\hspace{4mm}}
r@{\hspace{1.5mm}}r@{\hspace{4mm}}
r@{\hspace{1.5mm}}r@{\hspace{4mm}}
r@{\hspace{1.5mm}}r} 
\hline\hline%\\[-3.2mm]
$\lambda$(\AA) & ID & & 
\multicolumn{2}{c}{\#1} & 
\multicolumn{2}{c}{\#2} & \multicolumn{2}{c}{\#3} & 
\multicolumn{2}{c}{\#4}\\
& & & $F_{\lambda}$ & $I_{\lambda}$ & $F_{\lambda}$ & $I_{\lambda}$ & 
$F_{\lambda}$ & $I_{\lambda}$ & $F_{\lambda}$ & $I_{\lambda}$ \\[-3.4mm]\\
\hline
3727 & [O~{\sc ii}]        &    & 66.2  & 83.8 & 102.2 & 113.9 & 146.7 & 174.8 & 142.2 & 163.6 \\ 
3867 & [Ne~{\sc iii}]      &    & 40.6  & 50.1 & 57.6   & 62.6 &  10.1 & 11.8  & 183.6 &  204.7\\
3968 & [Ne~{\sc iii}] + H7 &    & 24.8  & 30.1 & 22.4   & 24.2 &  6.2  &  7.1  & 115.0 & 127.1 \\
4058 & N~{\sc iv}          & WR & 1.8   & 2.1   &   --  &  --  &  1.8  & 2.1   &  0.5  & 0.6   \\
4100 & H$\delta$            &    & 21.1  & 25.4 & 23.9  & 27.1  & 22.9  & 26.4  & 25.0  & 28.5 \\
4340 & H$\gamma$            &    & 41.4  & 46.4 & 45.9  & 49.9  & 42.3  & 45.5  & 42.8  & 46.4 \\
4363 & [O~{\sc iii}]       &    & 7.1   & 7.9  & 6.4   & 7.4   & 6.4   & 7.0   & 6.8   & 7.4  \\ 
4659 & [Fe~{\sc iii}]      &    & 0.41  & 0.43 & 0.47  & 0.49  & 6.3   & 6.5   & 0.57  & 0.59  \\
4686$^{\ast}$ & He~{\sc ii}         & WR & 8.5   & 8.9  & 2.1   & 2.2   & 
4.17  & 4.25  & 14.6  & 15.3 \\
4712 & [Ar~{\sc iv}]       &    & 2.0   & 2.1  & 1.5   & 1.5   & 0.96  & 0.99  & 1.2   & 1.2  \\
4741 & [Ar~{\sc iv}]       &    & 0.96  & 0.99 & 0.70  & 0.72  & 0.36  & 0.37  & 0.54  & 0.56  \\
4861 & H$\beta$             &    & 100   & 100  & 100   & 100   & 100   & 100   & 100   & 100  \\ 
4959 & [O~{\sc iii}]       &    & 213.8 & 206.3& 198.4 & 198.5 & 184.8 & 180.4 & 203.6 & 202.0 \\ 
5007 & [O~{\sc iii}]       &    & 630.0 & 604.0& 583.0 & 590.6 & 542.9 & 528.6 & 604.4 & 607.8 \\
5411 & He~{\sc ii}         & WR & 0.56  & 0.50 &  --   & --    &  --   &   --  &  1.16 & 1.15  \\
5808 & C~{\sc iv}          & WR &   --  &  --  & --   &  --   &  2.7   &  2.4  &   --  & --    \\
 5876 & He~{\sc i}          &    & 12.1  & 9.8  & 11.7 & 11.3  & 13.9   & 12.0  & 11.9  & 11.1 \\
\hline
H$\beta$                   &     &       & 0.44 & 1.12 & 0.39 & 0.49 & 0.44 & 0.86 & 0.13 & 0.20 \\
\hline
\multicolumn{3}{l}{$E(B-V)$} & 
\multicolumn{2}{c}{0.28 $\pm$ 0.05} & \multicolumn{2}{c}{0.08 $\pm$ 0.05} & 
\multicolumn{2}{c}{0.20 $\pm$ 0.05} & \multicolumn{2}{c}{0.12 $\pm$ 0.05} \\
\multicolumn{3}{l}{$T_{\rm e}$ (K)} &
\multicolumn{2}{c}{12~900 $\pm$ 700} & \multicolumn{2}{c}{12~700 $\pm$ 900} & 
\multicolumn{2}{c}{12~900 $\pm$ 700}  & \multicolumn{2}{c}{12~500 $\pm$ 400} \\
\multicolumn{3}{l}{O$^{+}$/H ($\times10^{-5}$)} &
\multicolumn{2}{c}{1.20 $\pm$ 0.07}  & \multicolumn{2}{c}{1.7 $\pm$ 0.1}   
&\multicolumn{2}{c}{2.5 $\pm$ 0.18}   & \multicolumn{2}{c}{2.6 $\pm$ 0.2}   \\
\multicolumn{3}{l}{O$^{2+}$/H ($\times10^{-5}$)} &
\multicolumn{2}{c}{10.3 $\pm$ 0.53}  
& \multicolumn{2}{c}{10.6 $\pm$ 0.61}  & 
\multicolumn{2}{c}{9.0 $\pm$ 0.65}   & \multicolumn{2}{c}{11.2 $\pm$ 0.87}  \\
\multicolumn{3}{l}{12 + $\log$(O/H)}  & \multicolumn{2}{c}{8.06 $\pm$ 0.02}  
& \multicolumn{2}{c}{8.09 $\pm$ 0.02}  &
\multicolumn{2}{c}{8.06 $\pm$ 0.03}  & \multicolumn{2}{c}{8.14 $\pm$ 0.03}  \\
\hline
\end{tabular}}
\par
$^\ast$ He~{\sc ii}  $\lambda$4686 fluxes are the sum of nebular and stellar components.
\end{table}