\begin{table}%t2
\caption{MIR fluxes for the Spitzer-IRAC sources towards the~mm core.
\label{spitz:tab}}
\small%\centerline
{
\begin{tabular}{l c c c c c c}
\hline\hline\noalign{\smallskip}
  ID  & \multicolumn{2}{c}{Position} &   $F_{\nu}(3.6)$    &
      $F_{\nu}(4.5)$   &   $F_{\nu}(5.8)$     &    $F_{\nu}(8.0)$   \\
      & $\alpha(2000)$ & $\delta(2000)$ & (mJy)   &  (mJy)  &  (mJy)
      &   (mJy)  \\
\hline\noalign{\smallskip}
   1  & $\rm 05^{h}40^{m}54.2^{s}$ & $35\degr41\arcmin59\arcsec$ &
         $8.6 \pm 0.8$  &  $7.0 \pm 0.8$    & $<$$12$ & $<$$39$ \\
   2  & $\rm 05^{h}40^{m}53.7^{s}$ & $35\degr41\arcmin56\arcsec$ &
         $7.8 \pm 0.9$  &  $4.7 \pm 1.2$ & $<$$11$ & $<$$19$ \\
   3  & $\rm 05^{h}40^{m}53.5^{s}$ & $35\degr41\arcmin53\arcsec$ &
        $17.2 \pm 0.3$  & $21.2 \pm 0.6$ &  $29 \pm 1$ &  $43 \pm 4$   \\
   4  & $\rm 05^{h}40^{m}53.7^{s}$ & $35\degr41\arcmin47\arcsec$ &
        $1.9 \pm 0.2$  &  $2.9 \pm 0.4$  & $<$$3$ & $<$$5$   \\
   5 (M~1) & $\rm 05^{h}40^{m}53.6^{s}$ & $35\degr41\arcmin43\arcsec$ &
        $8.6 \pm 0.1$  & $15.0 \pm 0.1$ &  $16 \pm 1$ &  $13 \pm 1$  \\
   6  & $\rm 05^{h}40^{m}54.0^{s}$ & $35\degr41\arcmin41\arcsec$ &
        $2.1 \pm 0.1$  &  $4.8 \pm 0.1$ &   $9 \pm 1$ &   $9 \pm 1$    \\
   7  & $\rm 05^{h}40^{m}54.4^{s}$ & $35\degr41\arcmin29\arcsec$ &
        $5.9 \pm 0.1$  &  $7.5 \pm 0.1$ &   $9 \pm 1$  &  $10 \pm 1$   \\
   8  & $\rm 05^{h}40^{m}53.8^{s}$ & $35\degr41\arcmin27\arcsec$ &
       $33.6 \pm 0.1$  & $33.1 \pm 0.1$ &  $36 \pm 1$ &  $54 \pm 1$    \\
  9$^a$  & $\rm 05^{h}40^{m}52.2^{s}$ & $35\degr41\arcmin41\arcsec$ &
        $5.0 \pm 0.3$    &  $4.7 \pm 0.2$ & $<$$5$ & $<$$24$  \\
  10  & $\rm 05^{h}40^{m}52.7^{s}$ & $35\degr41\arcmin45\arcsec$ &
        $8.5 \pm 0.2$  &  $7.6 \pm 0.2$ &   $9 \pm 1$ &  $18 \pm 7$     \\
  11  & $\rm 05^{h}40^{m}52.2^{s}$ & $35\degr41\arcmin55\arcsec$ &
        $5.4 \pm 0.8$  &  $2.9 \pm 0.7$ & $<$$17$ & $<$$95$  \\
  12  & $\rm 05^{h}40^{m}51.7^{s}$ & $35\degr41\arcmin57\arcsec$ &
        $3.5 \pm 0.8$  &  $2.7 \pm 0.6$ & $<$$20$ & $<$$59$   \\
  13 (S235AB-MIR) & $0\rm 5^{h}40^{m}53.4^{s}$ & $35\degr41\arcmin49\arcsec$ &
       $<$$0.6$ &   $5.0 \pm 0.3$ &  $14 \pm 1$ &  $28 \pm 2$ \\
  14  & $\rm 05^{h}40^{m}53.0^{s}$ & $35\degr41\arcmin53\arcsec$ &
        $1.7 \pm 0.9$  &  $3.7 \pm 1.0$  &  $3 \pm 4$ & $<$$35$      \\
  15  & $\rm 05^{h}40^{m}52.7^{s}$ & $35\degr41\arcmin52\arcsec$ &
        $2.4 \pm 1.1$  &  $1.2 \pm 0.9$ & $<$$9$ & $<$$22$   \\
\hline
\end{tabular}}
\smallskip
$^a$ N-E of a close by source only visible in the $5.8$~$\mu$m band.
\end{table}