\begin{table}%T2
%\centering
\par
\caption{Spectral and variability analyses of the brightest X-ray sources in the field of NGC~6383. The neutral hydrogen column density was frozen in the spectral fits at the interstellar value ($1.91 \times 10^{21}$~cm$^{-2}$). Columns 2 and 3 list the resulting best fit temperatures of the {\sc mekal} components, whilst column 4 provides the reduced $\chi^2$ along with the number of degrees of freedom. Columns 5 and 6 yield the observed and absorption corrected fluxes respectively. The quoted uncertainties correspond to formal errors on the spectral fits.\label{spec}}
\begin{tabular}{c c c c c c c}
\hline\hline
\#& $kT_1$ & $kT_2$ & $\chi^2_{\nu}$~(d.o.f.) & $f_{\rm X, obs}$ & $f_{\rm X, unabs}$ & Variability  \\
   & (keV)  & (keV)  &                          & ($10^{-13}$~erg~cm$^{-2}$~s$^{-1}$) & ($10^{-13}$~erg~cm$^{-2}$~s$^{-1}$) &\\
\hline 
16 & $\rm 0.87^{+0.23}_{-0.14}$ & $\rm 3.17^{+1.68}_{-0.97}$ & 1.08~(55) & 0.81 & 1.08 & No \\ 
50 & $\rm 0.61^{+0.24}_{-0.25}$ & $\rm 5.52^{+1.98}_{-1.31}$ & 1.02~(84) & 1.27 & 1.53 & Yes\\
55 & $\rm 0.33^{+0.34}_{-0.05}$ & $\rm 2.16^{+0.72}_{-0.43}$ & 1.18~(73) & 0.70 & 1.06 & No \\
65 & $\rm 0.73^{+0.13}_{-0.12}$ & $\rm 2.22^{+0.50}_{-0.38}$ & 1.04~(71) & 0.72 & 1.02 & No \\
\hline
\end{tabular}
\end{table}