\begin{table}%t1 
\caption{Point source fluxes.}\label{table:sourcelist}
%\centerline
 {
\begin{tabular}{r c c  r  r r r r r r r r r r r r  r}
\hline\hline\noalign{\smallskip}
ID & & & 2MASS designation & & & & & \multicolumn{4}{c}{\emph{Spitzer} fluxes and uncertainties$^a$} & & & & & SCUBA peak$^b$\\
 & RA& Dec  & $J$, $H$ \& $K_{\rm s}$ bands & 3.6~$\mu$m& $\sigma_{3.6}$& 4.5~$\mu$m & $\sigma_{4.5}$ & 5.8 $\mu$m & $\sigma_{5.8}$ & 8.0 $\mu$m & $\sigma_{8.0}$ & 24~$\mu$m & $\sigma_{24}$ & 70 $\mu$m$^c$ & $\sigma_{70}$ & sub-millimeter \\
 &  (J2000) & (J2000) & & (mJy) & (mJy) & (mJy) & (mJy) & (mJy) & (mJy) & (mJy) & (mJy) & (mJy) & (mJy) & (Jy) & (Jy)  \\
\hline
    S1 & 19$^{\rm h}$21$^{\rm m}$50$\fs$1 & +13$^\circ$47$\arcmin$57$\arcsec$ & -- &   $<$0.500  &   0.250   &   $<$0.500   &  0.250    &  $<$2.000  &   1.000 &     $<$2.000    & 1.000    & 26.647    &  3.033 & -- & -- & -- \\
    S2  & 19$^{\rm h}$21$^{\rm m}$50$\fs$2 & +13$^\circ$48$\arcmin$19$\arcsec$ & 19215022+1348185 &   2.994   &   0.518   &   6.248   &   0.854    &  8.012   &   1.115   &   3.862     & 1.107   & 101.585     & 7.051& -- & --	& P3   \\
   S3  & 19$^{\rm h}$21$^{\rm m}$53$\fs$0 & +13$^\circ$48$\arcmin$19$\arcsec$  & -- &  $<$0.500    & 0.250   &   $<$0.500    & 0.250    &  $<$2.000    & 1.000   &  $<$2.000    & 1.000     & 23.254     & 2.999 & -- & -- & -- \\
    S4  & 19$^{\rm h}$21$^{\rm m}$34$\fs$4 & +13$^\circ$49$\arcmin$12$\arcsec$ & 19213444+1349122 & 234.100   &   8.137   & 161.000  &  6.024  &  148.499  &   10.147  &   75.078  &   5.725  &   32.944   &   2.963 & -- & -- & -- \\
    S5  & 19$^{\rm h}$21$^{\rm m}$49$\fs$6 & +13$^\circ$49$\arcmin$31$\arcsec$ & --& 3.741    &  0.622   &  4.808     & 0.720   & 29.020     & 2.581   & 58.549    & 4.542   & 109.226    &  7.936 & 2.4 & 1.4 & part of P1 \\
    S6  & 19$^{\rm h}$21$^{\rm m}$50$\fs$2 & +13$^\circ$49$\arcmin$39$\arcsec$ & -- &$<$0.500    & 0.250    &  4.237    & 0.682    &  8.802     & 1.291     & 4.214     & 1.213    & 295.503   &  16.843 & 4.5 & 1.4 & part of P1  \\
    S7  & 19$^{\rm h}$21$^{\rm m}$40$\fs$7 & +13$^\circ$51$\arcmin$17$\arcsec$ & 19214073+1351176 & 1.233     & 0.314     & 1.581     & 0.352   &   $<$2.000    & 1.000     & $<$2.000    & 1.000    & 90.409     & 6.485 & -- & -- & --  \\
    S8  & 19$^{\rm h}$21$^{\rm m}$37$\fs$3 & +13$^\circ$51$\arcmin$23$\arcsec$ & 19213739+1351238 & 4.448    & 0.662    & 9.188     & 1.140   &  9.272    &  1.200    & 13.316    &  1.768   &  31.222    &  2.877 & -- & -- & --  \\
    S9  & 19$^{\rm h}$21$^{\rm m}$35$\fs$9 & +13$^\circ$52$\arcmin$01$\arcsec$ & 19213593+1352007 & 4.001    &  0.653    &  3.637     & 0.609    &  4.461     & 0.779    & 9.529     & 1.468    & 87.157    &  6.167 & -- & -- & --   \\
    S10  & 19$^{\rm h}$21$^{\rm m}$52$\fs$1 & +13$^\circ$52$\arcmin$24$\arcsec$  & -- &  $<$0.500    &  0.250    &  0.639    &  0.196     & $<$2.000    & 1.000     & $<$2.000    & 1.000    & 67.752    &  5.307 & -- & -- & -- \\
    S11 & 19$^{\rm h}$21$^{\rm m}$36$\fs$2 & +13$^\circ$52$\arcmin$21$\arcsec$  & -- & 0.201    & 0.122     & 1.109    &  0.293     & 1.206   &   0.429     & 1.988     & 0.959    & 24.073     & 2.446 & -- & -- & --  \\
    S12  & 19$^{\rm h}$21$^{\rm m}$45$\fs$6 & +13$^\circ$49$\arcmin$21$\arcsec$ & -- &  $<$0.500    & 0.250     & 0.260    & 0.133     & $<$2.000   &  1.000     & $<$2.000    & 1.000     & 13.778     & 2.018 & -- & -- & EP  \\
    S13 & 19$^{\rm h}$21$^{\rm m}$40$\fs$7 & +13$^\circ$50$\arcmin$55$\arcsec$ &  19214066+1350547 &  4.342    &  0.695     & 4.106    &  0.659     & 2.650     & 0.578     & $<$2.000    & 1.000    & 16.289     & 2.513 & -- & -- & --  \\
    S14 & 19$^{\rm h}$21$^{\rm m}$42$\fs$3 & +13$^\circ$50$\arcmin$21$\arcsec$ & 19214228+1350212 &  3.269     & 0.589     & 2.934    &  0.526     & 3.189     & 0.594     & 3.125     & 0.746     & 7.466     & 1.673 & -- & -- & --  \\
    S15  & 19$^{\rm h}$21$^{\rm m}$47$\fs$9 & +13$^\circ$49$\arcmin$20$\arcsec$ & -- &  $<$0.500    &  0.250 &   0.726 &  0.222 &  $<$2.000 &  1.000  & $<$2.000 &  1.000 & 2.757  & 0.918 & -- & -- & P2 \\
    S16 & 19$^{\rm h}$21$^{\rm m}$50$\fs$5 & +13$^\circ$47$\arcmin$28$\arcsec$ & -- &  3.303    &  1.331     & 2.624     & 1.304     & 6.388     & 0.908     & 2.290     & 0.687     & 5.544    &  1.381 & -- & -- & --  \\
    S17  & 19$^{\rm h}$21$^{\rm m}$48$\fs$7 & +13$^\circ$51$\arcmin$02$\arcsec$   & 19214875+1351034 &  212.300  &  7.346  &  111.500  & 4.275   &  81.086   &  6.043   &  41.064    &  3.503   &   7.142  &   1.262 & -- & -- & --  \\
    S18 & 19$^{\rm h}$21$^{\rm m}$48$\fs$1 & +13$^\circ$51$\arcmin$24$\arcsec$ & 19214807+1351249 & 436.200    & 18.300   & 240.600    & 14.500   & 87.205  &   6.401   & 87.228  &   6.439  &    13.605  &    1.598 & -- & -- & -- \\
    S19 & 19$^{\rm h}$21$^{\rm m}$49$\fs$4 & +13$^\circ$51$\arcmin$58$\arcsec$ & 19214945+1351581 & 416.400    & 18.690   & 233.300     & 9.739   & 69.551   &  5.225   & 88.545    & 6.542     & 12.832     & 1.589 & -- & -- & -- \\
    S20 & 19$^{\rm h}$21$^{\rm m}$40$\fs$8 & +13$^\circ$52$\arcmin$36$\arcsec$ & -- & 14.478   & 1.442    & 14.110     & 1.531    & 12.216    & 1.410    & 6.380     & 1.035    & 22.614    &  2.258 & -- & -- & -- \\
\hline
\end{tabular}}
\smallskip
$^a$ A ``$<$'' sign indicates that the corresponding flux value is an upper limit. The IRAC 3.6~$\mu$m and 4.5~$\mu$m fluxes and uncertainties for S4, S17 and S18 are taken from GLIMPSE. \\
$^b$ Sub-millimeter peaks~P1, P2 and EP are listed in Table~\ref{table:stages} of \citet{ormel2005}. See text in Sect.~\ref{sec:stageIobjects} for details of P1's subdivision. P3 is not defined in \citet{ormel2005}, its flux at 450 $\mu$m is estimated in Sect.~\ref{sec:stageIobjects} of the present study.\\
$^c$ The MIPSGAL mosaic shows one emission core of 6.9~Jy at the position of S5 and S6. See Sect.~\ref{sec:stageIobjects} for details of the subdivision of the MIPS 70~$\mu$m flux and Sect.~\ref{sec:SCUBAand2MASS} for the upper limit used for other sources.
\end{table}