\begin{table}%t1
 %%\centering

\par
\caption{\label{spc_class}Coordinates, LIRIS photometry and spectral classification of the selected objects within NGC~7538. }
\par
\begin{tabular}{c l l l c c c c c c c}
\hline\hline
%MOS Nr  &
Name &  ID & RA~(J2000) &    Dec~(J2000)   &  $J$ &  $H$ &  $K_{\rm s}$ &   $A_{\rm V}$(mag) &  Class. & ST  &   Notes \\
&     &      &      &      &      &      &      &      &      &      \\
\hline
IRS~6 &  &  23 13 34.3 & +61 30 14.3 &  8.71 $\pm$ 0.02\tablefootmark{\dag} & 8.21 $\pm$ 0.04$^{\dag}$ & 8.00 $\pm$ 0.01$^{\dag}$ & 5.4~$\pm$~0.4& &   O3$\pm$1V & O9~$\pm$~1V\tablefootmark{\ddag} \\
IRS~5 &  & 23 13 30.3 & +61 30 11.6 & 10.38~$\pm$~0.03$^{\dag}$ & 9.82~$\pm$~0.04$^{\dag}$ & 9.43~$\pm$~0.04$^{\dag}$ & 7.6~$\pm$~0.6&        &   O9~$\pm$~1V & O3~$\pm$~1V$^{\ddag}$ \\
\hline
%17 &
      & \#35  & 23  13  47.336   & +61  27  53.74 & 18.18~$\pm$~0.03 & 14.62~$\pm$~0.01 & 12.55~$\pm$~0.01 &35.0~$\pm$~0.2&           &   B1.5-B3V       &   \\
%9  &
      & \#25  & 23  13  43.820   & +61  29  28.37 & 13.41~$\pm$~0.01 & 12.33~$\pm$~0.01 & 11.83~$\pm$~0.02 &9.3~$\pm$~0.3&           &   B2-B7V     &   \\
%11 &
      & \#17  & 23  13  31.933   & +61  27  47.40 & 13.83~$\pm$~0.01 & 12.38~$\pm$~0.01 & 11.59~$\pm$~0.01 &13.6~$\pm$~0.2&           &   B5-B9V     &   \\
%16 &
      & \#63  & 23  13  45.058   & +61  27  53.88 & 18.13~$\pm$~0.05 & 15.14~$\pm$~0.03 & 13.18~$\pm$~0.01 &  --       & YSO       &     --       &   H$_2$   \\
%8  &
      & \#6   & 23  13  43.498   & +61  29  37.31 & 11.97~$\pm$~0.01 & 10.87~$\pm$~0.01 &  9.73~$\pm$~0.03 &  --       & YSO       &     --       &  neb \\
%19 &
      & \#14  & 23  13  44.538   & +61  27  15.19 & 14.89~$\pm$~0.02 & 12.81~$\pm$~0.02 & 11.39~$\pm$~0.01 &  --       & YSO       &     --       &  neb, Br-abs  \\
%4  &
      & \#11  & 23  13  30.688   & +61  29  07.47 & 17.50~$\pm$~0.04 & 13.78~$\pm$~0.01 & 11.15~$\pm$~0.01 &  --       & YSO       &     --       &  H$_2$, neb  \\
%5  &
 IRS~4 & \#2   & 23  13  32.219   & +61  29  07.32 & 11.40~$\pm$~0.01 & 10.43~$\pm$~0.05 &  9.43~$\pm$~0.09 &  --       & YSO       &     --       &  neb \\
%6  &
      & \#23  & 23  13  34.240   & +61  29  09.62 & 14.13~$\pm$~0.01 & 12.74~$\pm$~0.01 & 11.78~$\pm$~0.02 &  --       & FL        &     --       &   \\
%15 &
      & \#36  & 23  13  45.380   & +61  28  04.19 & 20.09~$\pm$~0.14 & 15.25~$\pm$~0.03 & 12.61~$\pm$~0.01 &           & FL        &     --       &   \\
%20 &
      & \#18  & 23  13  57.268   & +61  28  15.63 & 15.58~$\pm$~0.01 & 13.15~$\pm$~0.01 & 11.67~$\pm$~0.01 &  --       & FL        &     --       &    \\
%13 &
 IRS~3 & \#26  & 23  13  43.620   & +61  28  14.00 & 16.82~$\pm$~0.04 & 13.67~$\pm$~0.03 & 11.95~$\pm$~0.03 &29.7~$\pm$~0.7& \HII{}       &     --       &  \\
%7  &
      & \#12  & 23  13  33.537   & +61  28  49.80 & 15.72~$\pm$~0.07 & 12.92~$\pm$~0.07 & 11.10~$\pm$~0.04 &  --       & Herbig Be &     --       &     \\
%10 &
      & \#55  & 23  13  38.488   & +61  28  47.59 & 15.98~$\pm$~0.02 & 13.98~$\pm$~0.01 & 12.92~$\pm$~0.02 & 16.0~$\pm$~0.3& PMS       &   G9~$\pm$~1PMS       &   \\
%12 &
      & \#39  & 23  13  40.766   & +61  28  28.20 & 14.98~$\pm$~0.01 & 13.33~$\pm$~0.01 & 12.54~$\pm$~0.01 & 11.6~$\pm$~0.2& PMS       &   K1~$\pm$~1PMS      &   \\
%1  &
      & \#58  & 23  13  31.325   & +61  30  22.24 & 15.12~$\pm$~0.01 & 13.73~$\pm$~0.01 & 12.98~$\pm$~0.01 & 10.3~$\pm$~0.2& PMS       &   K1~$\pm$~1PMS      &  neb Br$\gamma$ \\
%3  &
      & \#41  & 23  13  33.391   & +61  29  35.77 & 14.43~$\pm$~0.01 & 13.15~$\pm$~0.01 & 12.56~$\pm$~0.01 &7.9~$\pm$~0.3&   PMS      &   K1~$\pm$~1PMS/III      &   \\
%18 &
      & \#15  & 23  13  57.238   & +61  27  47.40 & 14.95~$\pm$~0.01 & 12.60~$\pm$~0.01 & 11.56~$\pm$~0.01 &16.5~$\pm$~0.2&           &   G8~$\pm$~1III    &   \\
%2  &
      & \#46  & 23  13  34.218   & +61  30  17.64 & 14.18~$\pm$~0.07 & 13.03~$\pm$~0.09 & 12.66~$\pm$~0.08 &4.9~$\pm$~1.4&           &   KO~$\pm$~1III    &   \\
%14 &
      & \#60  & 23  13  44.280   & +61  28  10.10 & 15.68~$\pm$~0.01 & 13.91~$\pm$~0.01 & 13.05~$\pm$~0.03 &11.9~$\pm$~0.6&           &   K2~$\pm$~1III      &   H$_2$  \\
\hline
%   &
 IRS~7 & \#4   & 23  13  36.801   & +61  30  39.59  & 8.44~$\pm$~0.04$^{\dag}$ & 7.63~$\pm$~0.04$^{\dag}$ & 7.37~$\pm$~0.01$^{\dag}$ &2.6~$\pm$~0.6&         &    K0~$\pm$~1III       &  \\
\hline
\end{tabular}
\tablefoot{YSO: young stellar object; FL: featureless spectrum; PMS: pre-main-sequence. \tablefoottext{\dag}{Photometry from the 2MASS Point Source Catalog;}
\tablefoottext{\ddag}{classification by \cite{Russeil_07}}.}
\end{table}