\begin{table}%t2
%\centering
\par
\caption {\label{tab2}Summary of the stellar properties of the 8 RSGs for which accurate spectral classification was possible,
assuming a cluster distance of 6~kpc.}
  \begin{tabular}{lccccc}
        \hline \hline
        ID\# & $T_{{\rm eff}}$ & Spec & $A_{K}$ & $M_{K}$ &
        $\log(L_{{\rm bol}}/L_{\odot})$ \\
             & (K) & type &       &      &     \\
        \hline
 2 & $3605\pm147$ & M3 & $1.20\pm0.12$ &  $-9.34^{+0.39}_{-0.34}$ &   $4.51^{+0.14}_{-0.15}$ \\
 3 & $3535\pm125$ & M4 & $1.47\pm0.08$ & $-10.09^{+0.37}_{-0.33}$ &   $4.79^{+0.13}_{-0.15}$ \\
 4 & $3605\pm147$ & M3 & $1.44\pm0.12$ & $-10.12^{+0.39}_{-0.34}$ &   $4.82^{+0.14}_{-0.15}$ \\
 5 & $3660\pm130$ & M2 & $1.43\pm0.07$ &  $-9.85^{+0.37}_{-0.32}$ &   $4.73^{+0.13}_{-0.15}$ \\
 7 & $3790\pm130$ & M0 & $1.40\pm0.11$ &  $-9.11^{+0.38}_{-0.33}$ &   $4.48^{+0.13}_{-0.15}$ \\
 8 & $3840\pm175$ & K5 & $1.60\pm0.04$ &  $-9.23^{+0.36}_{-0.31}$ &   $4.54^{+0.12}_{-0.14}$ \\
 9 & $3790\pm130$ & M0 & $1.53\pm0.11$ &  $-9.14^{+0.38}_{-0.33}$ &   $4.49^{+0.13}_{-0.15}$ \\
10 & $3790\pm130$ & M0 & $1.60\pm0.11$ &  $-9.09^{+0.38}_{-0.33}$ &   $4.47^{+0.13}_{-0.15}$ \\
   \hline
   \end{tabular} 
\end{table}