\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}