\begin{table}%T2
        %\renewcommand{\arraystretch}{1.25}
        %\centering
\par
        \caption{Infrared flux densities of GRS~1915+105.
	$F_{\rm obs}$ is the observed flux directly measured on
	ISOCAM images, except for the $J$, $H$ and $K$~band fluxes which were
	reported from \citet{mahoney} and transformed into mJy units.
	$F_{\rm der}$ is the resulting flux after dereddening with two
	different laws: from \citet{lutz96} and from \citet{draine89}.}
	\label{tabfluxGRS1915}
 \begin{tabular}{lc@{~}cc@{~}cc@{~}c}
\hline
\hline
Filter & \multicolumn{2}{c}{$F_{\rm obs}$ (mJy)} & \multicolumn{2}{c}{$F_{\rm der}$ Lutz (mJy)} & \multicolumn{2}{c}{$F_{\rm der}$ Draine (mJy)} \\
	& 1996 & 1997 & 1996 & 1997 & 1996 & 1997 \\
\hline
$LW$1 (4--5~$\mu$m) &	$11.2\pm 3.4$ &      	      & $42.1\pm 13$ &      	& $19.2\pm 5.8$ &      \\
$LW$2 (5--8.5~$\mu$m) &	$5.39\pm 1.6$ & $9.77\pm 2.9$ & $17.4\pm 5.2$ & $31.5\pm 14$ & $7.72\pm 2.3$ & $14.0\pm 4.2$ \\
$LW$4 (5.5--6.5~$\mu$m) &	     	      & $11.6\pm 3.5$ & 	   & $37.1\pm 11$ & 	     & $16.0\pm 4.8$ \\
$LW$6 (7--8.5~$\mu$m) &	     	      & $11.9\pm 3.6$ & 	   & $38.4\pm 12$ & 	     & $19.5\pm 5.9$ \\
$LW$7 (8.5--10.7~$\mu$m) &	$1.53\pm 0.5$ & $4.87\pm 1.5$ & $7.37\pm 2.2$ & $23.5\pm 7.0$ & $7.26\pm 2.2$ & $23.1\pm 6.9$ \\
$LW$8 (10.7--12~$\mu$m) &	$3.54\pm 1.1$ & $6.58\pm 2.0$ & $10.3\pm 3.1$ & $19.2\pm 5.8$ & $10.8\pm 3.2$ & $20.1\pm 6.0$ \\
$LW$9 (14--16~$\mu$m) &	     	      & $13.8\pm 4.1$ & 	   & $23.9\pm 7.2$ & 	     & $24.0\pm 7.2$ \\
$LW$3 (12--18~$\mu$m) &	$5.34\pm 1.6$ & $10.5\pm 3.1$ & $9.25\pm 2.8$ & $18.2\pm 5.5$ & $9.29\pm 2.8$ & $18.3\pm 5.5$ \\
$LW$10 (8--15~$\mu$m) &	    	      & $14.7\pm 4.4$ &	  	   & $41.3\pm 12$	&	     & $36.0\pm 11$ \\
$J$ (1.25~$\pm$~0.15~$\mu$m) &	$0.688\pm 0.04$ &  & $121.0\pm 7.8$ & & $135.2\pm 8.7$ & \\
$H$ (1.65~$\pm$~0.15~$\mu$m) &	$3.14\pm 0.14$ &   & $78.3\pm 3.6$ & & $77.1\pm 3.6$ & \\
$K_{\rm s}$ (2.15~$\pm$~0.15~$\mu$m) & $6.98\pm 0.26$ &   & $52.7\pm 1.9$ & & $51.8\pm 1.9$ & \\
\hline
\end{tabular}
        \end{table}