\begin{table}%t3
\caption{\label{Tableflux}Integrated flux densities measured with {\it {2MASS}}, \iras, \spitz\ and~\lab.}
\par
\small%\centerline
 {
\begin{tabular}{cp{2.6cm}cp{3mm}cp{3mm}cp{3mm}cp{3mm}c}
\hline
\hline
\noalign{\smallskip}
&&&& NGC 1705 && Haro 11 && Mrk 1089	&& UM 311 system  \\
\hline
2MASS &1.25 \mic\ flux density &(in mJy) && 52 $\pm$ 1.6	&& 13  $\pm$ 0.3  	&& 12.2 $\pm$ 0.6	&& 12.8 $\pm$ 1 \\
2MASS &1.65 \mic\ flux density &(in mJy) && 50.9 $\pm$ 2	&& 13 $\pm$ 0.5 	&& 13.9 $\pm$ 0.9	&&  12.6 $\pm$ 1 \\
2MASS &2.17 \mic\  flux density &(in mJy) && 41.1 $\pm$ 2.4	&& 13.8 $\pm$ 0.7 	&& 12.2 $\pm$ 1.2	&& 11.5 $\pm$ 1  \\
IRAC &3.6 \mic\  	flux density &(in mJy) && 26.3 $\pm$ 3	&& 22.5 $\pm$ 2 	&& 14.9 $\pm$ 2	&& ...   \\
IRAC &4.5 \mic\ 	flux density &(in mJy) && 17.9 $\pm$ 2	&& 28.9 $\pm$ 3 	&& 11.2 $\pm$ 1	&& 5.5 $\pm$ 0.5   \\
IRAC &5.8 \mic\ 	flux density &(in mJy) && 16 $\pm$ 2		&& 72.7 $\pm$ 7 	&& 33.3 $\pm$ 3	&& ...   \\
IRAC &8 \mic\ flux density &(in mJy) && 17.9 $\pm$ 2	&& 177 $\pm$ 18 	&& 92.5 $\pm$ 9	&& 35.6 $\pm$ 4   \\
IRAS  &12 \mic\ flux density &(in mJy) &&  ...			&& 417 $\pm$ 46 	&& 106 $\pm$ 21	&& ...   \\
MIPS &24 \mic\ flux density &(in mJy) && 52.7 $\pm$ 5	&& 1930 $\pm$ 193 && 460 $\pm$ 46	&& 151 $\pm$ 15   \\
IRAS &25 \mic\ flux density &(in mJy) && ...				&& 2500 $\pm$ 25 	&& 579 $\pm$ 29	&& ...  \\
IRAS &60 \mic\  flux density &(in mJy) && 868 $\pm$ 61	&& 6880 $\pm$ 41 	&& 4010 $\pm$ 40	&& ...  \\
MIPS &70 \mic\ 	flux density &(in mJy) && 1113 $\pm$ 222	&&  4190 $\pm$ 838 && 3993 $\pm$ 798 && 1476 $\pm$ 148 \\
IRAS &100 \mic\ 	flux density &(in mJy) &&  1610 $\pm$ 100	&& 4730 $\pm$ 640	&&  5430 $\pm$ 181&& ...  \\
MIPS &160 \mic\  flux density &(in mJy) && 1115 $\pm$ 222	&& 1663 $\pm$ 332 	&& ...				&& ...  \\
LABOCA$^a$ &870 \mic\  flux density &(in mJy) && 114 $\pm$ 17	&& 40 $\pm$ 6 		&& 67.4 $\pm$ 10.1	&& 32.2 $\pm$ 7    \\
\hline
\end{tabular}}
\medskip
$^a$ The 10$\%$ non-dust contamination was subtracted from the \lab\ flux densities.
\vspace*{5mm}
\end{table}