\begin{table}%t9
\caption{\label{table:flux}Source fluxes including IRAC~1-4, MIPS~1-2, SHARC-II, SCUBA and 1.3~mm data.}
\par
\small%\centerline
 {
\begin{tabular}{l c c c c c c c c c c c}
 \hline \hline 
Source  	&3.6 $\mu$m$^e$&4.5 $\mu$m$^e$&5.8 $\mu$m$^e$&8.0 $\mu$m$^e$&24 $\mu$m$^e$&70 $\mu$m&350 $\mu$m&450 $\mu$m&850 $\mu$m&850 $\mu$m&1300 $\mu$m\\
                & IRAC I&IRAC II&IRACIII&IRAC IV& MIPS I&MIPS II &SHARC & SCUBA & SCUBA& SCUBA& \\
                &       &       &       &       &       &$\sim$10$''$& 9--25$''$$^b$& 10 $''$$^b$ &15$''$& 25$''$& 15$''$ \\
	        & mJy   &mJy    &mJy    &mJy    &mJy    &mJy     &mJy      &  mJy   &  mJy      &   mJy   &  mJy        \\ 
\hline
C2D-162527.6    & 1.15e1& 1.77e1& 3.00e1& 6.03e1& 8.51e1& --      &   --     & --        &  $<$3e1    & $<$3e1   & \\
GSS 26	        & 2.86e2K& 3.86e2K& 5.09e2& 6.17e2& 7.98e2& --      &         & 6.5e2      &  3.0e2$^b$  & 1.6e3    & 1.e2\\
CRBR 2315.8-1700& 4.53e1& 8.77e1& 1.61e2& 2.37e2& 5.16e2& --      &   --     &          & 2.1e2       & 7.5e2     & 8.5e1)\\
CRBR 2317.3-1925& 1.05e1& 1.15e1& 1.39e1& 2.05e1& 1.46e1& --      &         &          &1.5e2$^b$    & 1.7e2     &\\
VSSG 1	        & 7.57e2& 1.01e3& 9.67e2& 9.96e2& 9.48e2& --      &         & $<$6.7e2  &2.4e2$^b$    & 3.0e2     &5e1\\
GSS 30	        & 1.06e3& 2.27e3& 4.1e3 & 5.4e3 & --	& 7.83e4 &2.5e3$^a$ & 1.4e3     & 2.2e2$^b$   & 3.2e2    & 9e1\\
LFAM 1	        & 1.28e1& 1.82e1*& 3.78e1& 1.59e1*& 2.41e2*& 6.31e4 &         & 2.7e3     & 5.7e2$^b$   & 2.6e3    & 1.1e3\\
CRBR 2324.1-1619     & 9.37e0& 1.59e1& 2.17e1& 2.95e1& 4.47e2& --      &         &          & 8.4e2       & 6.1e3    &\\
VLA 1623        &  --	& 1.57e-1*&2.45e-1*& --	& 4.04e1& --      &4e5$^c$  &3.9e5$^c$ & 5.0e3      & 1.7e4   & 1.2e3\\
GY51            & 2.86e2& 3.71e2& 4.38e2& 4.66e2& 6.39e2*& --      &         &          & 3.3e2       & 1.7e3    & 2e1\\
CRBR 2339.1-2032          & 3.04e1&4.48e1 & 6.05e1& 8.28e1& 3.93e2& --      &         &          & 8e1        & 3e2     &3e2\\
WL 12	        & 2.39e2&7.44e2 & 1.61e3& 2.24e3&   --	& 7.0e3  &6.7e3$^a$ & 7.5e2      & 2.2e2$^b$   & 7.1e2     & 1.2e2\\
WL 2            & 7.92e1&1.11e2 & 1.28e2& 1.48e2& 4.46e2& --      &         &          & 4e1        & 1.4e2     & 3e1\\
LFAM 26         & 6.11e0&1.07e1 & 1.66e1& 2.96e1& 4.59e2& --      &         &          & 2.2e2       & 6.9e2     & 1e2\\
WL 17	        &  2.4e2&4.16e2 & 5.53e2& 6.95e2&2.79e3 & 6.8e3  &         & $<$8.7e2   & 1e2$^b$   & 6.1e2     & 7.5e1\\
Elias 29        &  --	& --	& 1.28e4&  --	& --	&$<$4.7e4&4.3e3$^a$ & 2.0e3     & 4.1e2$^b$   & 9.4e2     & 9.5e1\\
GY 224	        & 2.03e2&3.05e2K &3.58e2 & 3.67e2& 9.07e2&        &         &          & 1.3e2       & 3.7e2     & 5e1\\
 WL19           & 2.15e2&3.54e2K & 4.06e2& 3.28e2&2.23e2 & --      &         &          & 2.0e2       & 8.3e2     & 3e1\\
WL 20S	        & 6.53e-1*$^d$&2.97e1& 3.74e1*& 2.43e2&1.46e2* & 1.4e4 & 8.2e2$^a$& 4.0e2      & 1.8e2$^b$   & 6.0e2     & 4.7e1\\
IRS 37	        & 1.27e2& 2.06e2& 2.86e2& 2.68e2& 7.8e2 & 1.4e4  &         & $<$5.9e2  & 9.3e1$^b$    & 3.0e2     & $<$1e1\\
WL 3            & 9.86e1& 1.63e2& 2.08e2& 2.04e2& 3.25e2&$<$2.4e4&         & $<$5.8e2  & 1.2e2$^b$   & 4.4e2     & $<$6e1\\
IRS 42	        & 1.06e3& 1.63e3& 2.1e3 & 2.98e3& 3.45e3& 3.0e3  &1.5e3$^a$ &          & 1.7e2       & 7.3e2     & $<$6e1\\
WL 6	        & 4.67e2K& 9.25e2& 1.44e3& 1.73e3& 4.36e3& 3.5e3  &         & 1.4e2      &$<$3e1      & $<$3e1   & $<$2e1\\
GY 256	        & 1.09e1& 1.19e1& 1.38e0*& 8.58e-1*&2.86e1*& 3.5e3  &         &          &  $<$3e1    & $<$3e1   &\\
IRS 43	        & 6.29e2& 1.24e3& 1.79e3& 2.19e3& --	& 2.4e4  & 2.1e3$^b$& 1.8e3     &  2.5e2$^b$  & 2.7e3    & 8e1\\
IRS 44	        & 7.31e2& 1.83e3& 2.94e3& 2.32e3& --	& 2.5e4  &         &          & 3.6e2       & 1.2e3    & 6e1\\
Elias 32        & 1.87e2& 2.72e2& 3.82e2& 4.81e2& 7.12e2& 1.1e4  &         &          & 1.7e3      & 6.4e3    & $<$5e1\\
Elias 33        & 7.4e2 & 1.19e3& 1.58e3& 2.04e3& 1.72e3&$<$1.0e4&4.4e3$^a$ &          & 1.2e3      & 4.4e3    &$<$2e1\\
IRS 48	        & 1.41e3& 1.6e3 & 4.06e3& 6.0e3 & --	& 1.7e4  &         & $<$1.6e3 & 1.8e2$^b$   & 1.9e2     & 6e1\\
GY 312          & 1.58e1& 2.67e1& 3.82e1& 5.32e1& 4.61e2& 7.1e2  &         &          & $<$3e1     & $<$3e1   &\\
IRS 51	        & 7.52e2& 9.16e2& 1.00e3& 1.07e3& 2.73e3& 2.4e3  &1.4e3$^a$ &  $<$6.8e2 & 2.2e2       & 7.8e2     &1.1e2\\
C2D-162741.6    & 8.31e0& 1.39e1& 2.04e1& 2.86e1& 6.89e1& 5.3e2  &         &          & 1e2       & 3.5e2     &\\
C2D-162748.2    & 1.21e0& 2.21e0& 3.64e0& 1.41e1& 1.84e2&        &         &          & 5e1        & 6e1      &\\
IRS 54	        & 5.25e2K& 7.12e2& 9.31e2& 1.01e3& 3.56e3& 5.0e3  &         &          & 1e2       & 3.2e2     & 3e1\\
IRAS 16285      & 5.89e-1&2.55e0& 4.49e0K& 3.13e0& 9.01e1& 1.7e3  &         &          & 5e2       & 1.6e3    &\\
C2D-162857.9    & 9.73e0 &1.7e1 &2.57e1 & 3.83e1& 1.61e2& --      &         &          & 5e1        & 8.5e2     &\\
IRS 63	        & 5.89e2& 9.57e2& 1.25e3& 1.45e3& 3.23e3& 8.3e3  &6.7e3$^b$ & 4.7e3     & 1.0e3$^b$  & 2.4e3    & 3.7e2\\ 
\hline
\multicolumn{12}{c}{\textbf{Disks}}  \\ 
Haro 1-4        & 5.19e2& --     & 3.73e2& --     & 8.39e2& 5.6e2  &         &          &   -- & --      &\\
DoAR 25	        & 3.67e2& 2.92e2& 2.99e2& 2.58e2&3.99e2 & 1.4e3  &         &          & 4.6e2$^b$   &5.2e2      & 2.8e2\\
OphE MM3        & 1.42e0&1.79e0 & 1.88e0*& 2.22e0& 1.41e0*& --      &1.6e3$^a$ & 5.4e2      & 1.6e2       & 3.6e2     & \\
SR 21           & 1.3e3 & 1.17e3& 1.28e3& 1.66e3& --     & 1.3e3  & 2.8e3$^b$& 1.9e3     & 4.0e2$^b$   &4.7e2      & 9.5e1\\
CRBR 2422.8-3423& 5.4e1 & 1.31e2& 1.91e2& 1.98e2& 1.34e3& 9.8e3  &         &          & 1.3e3      & 3.2e3    & 1.5e2\\
IRS 46	        & 1.72e2K& 2.71e2& 4.02e2& 4.11e2& 6.39e2*& --      &1.4e3$^a$ &          & 1.8e2       & 5.1e2     & 4.5e1\\
SR 9            & 7.84e2& 5.75e2& 4.65e2& 4.84e2& 1.04e3& --      &         &          &  $<$25$^b$&2.9e1& 1.5e1\\ 
2Mass 16282     & 2.32e0& 2.00e0& 1.39e0& 8.15e-1&1.58e0& --      &  9e1$^b$ & 8e1       & 5.8e1        & 2.7e2\\
\hline 
\end{tabular}}
\medskip
$^a$ This paper;
$^b$ 350/450~$\mu$m flux taken from \citet{Andrews07}. Fluxes obtained with SHARC-II are given either in a~9$''$~beam \citep{Andrews07} or in a~25$''$~radius (This work); 
$^c$~data taken from \citet{Andre93};
$^d$~two sources within 4$''$ with a total flux of 2e2~mJy;
$^e$~IRAC and MIPS-24 Fluxes marked with ``$*$'' are band-filled sources with a~$S/N$~$<$~5 or sources with $S/N$~$<$~5. Such limits are caused either by saturation or a very low emission. A~``K'' added to the flux indicates that the obtained flux was flagged as ``Complex'', with multiple detection within~2$-$3$''$.
\end{table}