Table 2: 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 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.
# kT1 kT2 $\chi^2_{\nu}$ (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)  
16 $\rm0.87^{+0.23}_{-0.14}$ $\rm 3.17^{+1.68}_{-0.97}$ 1.08 (55) 0.81 1.08 No
50 $\rm0.61^{+0.24}_{-0.25}$ $\rm 5.52^{+1.98}_{-1.31}$ 1.02 (84) 1.27 1.53 Yes
55 $\rm0.33^{+0.34}_{-0.05}$ $\rm 2.16^{+0.72}_{-0.43}$ 1.18 (73) 0.70 1.06 No
65 $\rm0.73^{+0.13}_{-0.12}$ $\rm 2.22^{+0.50}_{-0.38}$ 1.04 (71) 0.72 1.02 No


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