\begin{table}%t2
\caption{Observed fluxes and magnitudes of the Superantennae. Optical and IRAS
data,  from Mirabel et~al. (\cite{mirabel1991}), are in the first thirteen rows, the next six rows report
the ISOCAM LW bands fluxes by Charmandaris et~al. (\cite{charmandaris2002}) and finally Klaas et~al. (\cite{klaas2001}) measurements are
in the last eleven rows; the 1300~$\mu$m datum was obtained with SEST, while the others
with ISOPHOT. Infrared observations marked with $^*$ have been splitted
between the two nuclei, by means of a procedure 
described in the text. Integrated IR fluxes
were obtained from IRAS data through Sanders \& Mirabel (\cite{SM96}) calibration and are expressed in W~m$^{-2}$.}
%%\centering
\par
\begin{tabular}{c *{3}{c}}
\hline
\hline
		& South	8$''$& North 8$''$	& Global \\
\hline
$B$		&0.365 mJy&0.324 mJy& 1.401 mJy 	\\
$V$		&0.880 mJy&0.687 mJy& 2.997 mJy 	\\
$R$		&1.397 mJy&0.949 mJy& 4.220 mJy	\\
$I$		&2.052 mJy&1.407 mJy& 6.197 mJy	\\
$J$		&3.544 mJy&2.664 mJy&  --	\\
$H$		&5.720 mJy&3.353 mJy&  --	\\
$K$		&7.586 mJy&3.467 mJy&  --	\\
$L$		&20.79 mJy&2.117 mJy&  --	\\
$N$		&110.6 mJy&23.76 mJy&  --	\\
$S(12~\mu{\rm m})$	&0.210$^*$  Jy&0.012$^*$  Jy& 0.222  Jy \\
$S(25~\mu{\rm  m})$	&1.217$^*$  Jy&0.025$^*$  Jy& 1.242  Jy \\
$S(60~\mu {\rm m})$	&5.370$^*$  Jy& -- & 5.484  Jy \\
$S(100~\mu{\rm  m})$	&5.671$^*$  Jy& -- & 5.789  Jy \\
\hline
$S(6~\mu{\rm  m})$	& 0.0900 Jy & 0.0019 Jy & 0.0919 Jy \\
$S(6.75~\mu{\rm  m})$	& 0.1069 Jy & 0.0048 Jy & 0.1117 Jy \\
$S(7.75~\mu{\rm  m})$	& 0.1501 Jy & 0.0083 Jy & 0.1584 Jy \\
$S(9.62~\mu{\rm  m})$	& 0.0912 Jy & 0.0051 Jy & 0.0963 Jy \\
$S(11.4~\mu{\rm  m})$	& 0.1075 Jy & 0.0059 Jy	& 0.1134 Jy \\
$S(15~\mu{\rm  m})$	& 0.2840 Jy & 0.0059 Jy & 0.2899 Jy \\
\hline	
$S(10~\mu{\rm  m})$	& 0.116$^*$ Jy & 0.007$^*$ Jy & 0.123 Jy \\
$S(12~\mu{\rm  m})$	& 0.189$^*$ Jy & 0.011$^*$ Jy & 0.200 Jy \\
$S(15~\mu{\rm  m})$	& 0.392$^*$ Jy & 0.008$^*$ Jy & 0.400 Jy \\
$S(25~\mu{\rm  m})$	& 1.293$^*$ Jy & 0.027$^*$ Jy & 1.320 Jy \\
$S(60~\mu{\rm  m})$	& 5.456$^*$ Jy & -- & 5.570 Jy \\
$S(90~\mu{\rm  m})$	& 5.153$^*$ Jy & -- & 5.260 Jy \\
$S(120~\mu{\rm  m})$	& 4.183$^*$ Jy & -- & 4.270 Jy \\
$S(150~\mu{\rm  m})$	& 2.998$^*$ Jy & -- & 3.060 Jy \\
$S(180~\mu{\rm  m})$	& 2.253$^*$ Jy & -- & 2.300 Jy \\
$S(200~\mu{\rm  m})$	& 1.577$^*$ Jy & -- & 1.610 Jy \\
$S(1300~\mu{\rm  m})$	& 0.011$^*$ Jy & -- & 0.012 Jy \\
\hline
$S_{{\rm IR}}$	&5.205 $\times$ $10^{-13}$ &1.26 $\times$ $10^{-14}$  &5.28 $\times$ $10^{-13}$\\
\hline
\end{tabular}
\label{tab:fluxes_nuclei}
\end{table}