\begin{table}%t2
%\centering
\par
\caption{\label{Integrated_fluxes}Continuum fluxes integrated over the envelope of each source and used in the SED analysis.}
\begin{tabular}{llllll}
\hline \hline \noalign{\smallskip}
Source  &   CB3 & Cep E       & IC1396 N    & NGC7129     & Serpens     \\ 
&mm   &mm          & BIMA 2      & FIRS 2      & FIRS~1 \\
\hline 
$F_{24~\mu {\rm m}}$ (Jy) -- Spitzer   & $1.4\pm0.8$ & $6.0\pm3.0$ & $2.3\pm2.0$ & $6.0\pm3.0$ & $3.0\pm1.0$ \\ 
$F_{60\mu {\rm m}}$ (Jy) -- IRAS   & $31\pm15$   & $61\pm30$   & --           & --   & --           \\ 
$F_{70~\mu {\rm m}}$ (Jy) -- Spitzer   & $58\pm20$   & $100\pm40$  & --           & $110\pm60$  & $135\pm50$  \\ 
$F_{100~\mu {\rm m}}$ (Jy) -- IRAS   & $110\pm55$  & $110\pm55$  & --           & --           & --           \\ 
$F_{450~\mu {\rm m}}$ (Jy) -- JCMT & $30\pm10$   & $44\pm10$   & $100\pm30$  & $80\pm40$   & $130\pm40$  \\ 
$F_{850~\mu {\rm m}}$ (Jy) -- JCMT  & $2.0 \pm 1.0$ & $4.1\pm1.3$ & $17\pm7.0$  & $4.8\pm2.0$ & $14\pm4.0$  \\ 
F$_{1300~\mu {\rm m}}$ (Jy) -- IRAM30~m  & -- & $1.0\pm0.2$ & -- & $2.2\pm0.5$ & --           \\
\hline
\end{tabular}
\vspace*{-1mm}
\end{table}