\begin{table}%t3
\caption{X-ray spectral fits of \tr~sources. The complete version is available in the electronic version.}
\label{xspectab}
\par
\small%\centerline
 {
\begin{tabular}{lllllll}
\hline \hline
\multicolumn{1}{l}{$N_{x}$} &
\multicolumn{1}{l}{Cnts.} &
\multicolumn{1}{l}{{Stat.}} &
\multicolumn{1}{l}{$\log~(N_{\rm H}$)} &
\multicolumn{1}{l}{$kT$} &
\multicolumn{1}{l}{$\log~(L_{\rm x})$} &
\multicolumn{1}{l}{{flag}} \\
\multicolumn{1}{l}{\#} &
\multicolumn{1}{l}{(ph)} &
\multicolumn{1}{l}{($\chi^2_\nu$)} &
\multicolumn{1}{l}{(cm$^{-2}$)}&
\multicolumn{1}{l}{(keV)}&
\multicolumn{1}{l}{(erg/s)} &
\multicolumn{1}{l}{} \\
\hline
   1 &     30 &   $--$ &    $-----$ &   $-----$ & 30.51 &       no-fit  \\
   2 &     36 &   $--$ &    $-----$ &   $-----$ & 30.58 &       no-fit  \\
   3 &    208 &  0.66 &  22.01  $\pm$  0.16 &  2.07  $\pm$  0.56 & 31.58 &	 fitted  \\
   4 &     55 &  0.94 &  21.90  $\pm$  0.31 &  2.96  $\pm$  2.61 & 30.50 &	 fitted  \\
   5 &     28 &   $--$ &    $-----$ &   $-----$ & 30.48 &       no-fit  \\
   6 &     41 &   $--$ &    $-----$ &   $-----$ & 30.64 &       no-fit  \\
   7 &     47 &   $--$ &    $-----$ &   $-----$ & 31.29 &{\tiny Tr16-19}\\
   8 &     54 &   $--$ &    $-----$ &   $-----$ & 30.76 &       no-fit  \\
   9 &     45 &   $--$ &    $-----$ &   $-----$ & 30.68 &       no-fit  \\
  10 &     25 &   $--$ &    $-----$ &   $-----$ & 30.42 &       no-fit  \\
  11 &     41 &   $--$ &    $-----$ &   $-----$ & 30.72 &       no-fit  \\
  12 &    132 &  1.50 &  21.23  $\pm$  0.62 &  2.65  $\pm$  0.94 & 31.08 &	 fitted  \\
  13 &     89 &  0.40 &  21.64  $\pm$  0.14 &  0.67  $\pm$  0.93 & 30.83 &	 fitted  \\
  14 &     15 &   $--$ &    $-----$ &   $-----$ & 30.23 &       no-fit  \\
  15 &     41 &   $--$ &    $-----$ &   $-----$ & 30.65 &       no-fit  \\
  16 &     23 &   $--$ &    $-----$ &   $-----$ & 30.40 &       no-fit  \\
  17 &     28 &   $--$ &    $-----$ &   $-----$ & 30.48 &       no-fit  \\
  18 &     31 &  0.80 &  22.32  $\pm$  0.32 &  1.36  $\pm$  0.88 & 31.04 &       fitted  \\
  19 &      7 &   $--$ &    $-----$ &   $-----$ & 29.93 &       no-fit  \\
  20 &     30 &   $--$ &    $-----$ &   $-----$ & 30.51 &       no-fit  \\
  21 &     25 &  1.21 &  21.97  $\pm$  0.65 &  0.29  $\pm$  0.18 & 30.02 &	 fitted  \\
  22 &    176 &  0.94 &  21.81  $\pm$  0.22 &  3.32  $\pm$  1.45 & 31.46 &	 fitted  \\
  23 &     25 &   $--$ &    $-----$ &   $-----$ & 30.43 &       no-fit  \\
  24 &     22 &   $--$ &    $-----$ &   $-----$ & 30.38 &       no-fit  \\
  25 &    177 &  1.87 &  22.00  $\pm$  0.18 &  2.17  $\pm$  0.74 & 31.52 &	 fitted  \\
  26 &     44 &  0.90 &  21.70  $\pm$  0.27 &  1.49  $\pm$  0.54 & 30.38 &	 fitted  \\
  27 &     51 &  0.50 &  22.06  $\pm$  0.32 &  2.11  $\pm$  1.27 & 31.03 &	 fitted  \\
  28 &     77 &  0.47 &  21.28  $\pm$  0.72 &  1.49  $\pm$  0.44 & 30.83 &	 fitted  \\
  29 &     36 &   $--$ &    $-----$ &   $-----$ & 30.59 &       no-fit  \\
  30 &     12 &   $--$ &    $-----$ &   $-----$ & 30.12 &       no-fit  \\
\hline
\end{tabular}}
\medskip
Notes: last column flag: sources with no spectral information ({\sc no-fit}) have their X-ray luminosities computed by using an average count-rate to \Lx\ conversion factor (see
Sect.~\ref{lx}). ``H{\sc ard tail}'' flag refers to the need of more components in the spectral models. Spectral fit parameters for OB-type stars are not listed here as they are presented in Table~\ref{ob}.
\end{table}