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Table 5:

Results of the fit to the individual X-ray spectra of models of the kind wabs1$\ast $mekal+wabs2$\ast $powerlaw.
No. Phase $N_{{\rm H1}}$ kT1 Norm1 $N_{{\rm H2}}$ Ph.I. Norm2 $\chi_{\nu}^{2}$ d.o.f.
    (1022 cm-2) (keV) (10-4 cm-5) (1022 cm-2)   (10-4 cm-5)    
II+VI 0.582/0.680 $\rm0.37^{+0.11}_{-0.16}$ $\rm0.59^{+0.03}_{-0.03}$ $\rm 1.51^{+0.57}_{-0.46}$ $\rm0.30^{+0.40}_{-0.15}$ $\rm 2.47^{+0.42}_{-0.18}$ $\rm0.76^{+0.49}_{-0.26}$ 1.20 285
VII 0.765 $\rm0.50^{+0.08}_{-0.20}$ $\rm0.60^{+0.04}_{-0.04}$ $\rm 1.93^{+0.42}_{-0.90}$ $\rm 1.28^{+1.30}_{-0.89}$ $\rm 3.01^{+0.36}_{-0.66}$ $\rm 1.57^{+3.23}_{-0.77}$ 1.07 124
III 0.828 $\rm0.67^{+0.14}_{-0.14}$ $\rm0.58^{+0.05}_{-0.05}$ $\rm 2.15^{+1.25}_{-1.01}$ $\rm0.74^{+0.69}_{-0.60}$ $\rm 3.21^{+0.24}_{-0.72}$ $\rm 2.01^{+1.25}_{-1.27}$ 1.34 116
IV 0.903 $\rm 1.11^{+0.06}_{-0.30}$ $\rm0.61^{+0.07}_{-0.06}$ $\rm 5.72^{+1.98}_{-2.95}$ $\rm 4.16^{+9.83}_{-4.53}$ $\rm 3.01^{+2.76}_{-2.31}$ $\rm 2.13^{--}_{--}$ 1.08 76
V 0.994 $\rm 1.58^{+0.26}_{-0.26}$ $\rm0.71^{+0.19}_{-0.12}$ $\rm 5.01^{+2.57}_{-2.03}$ $\rm 7.08^{+7.17}_{-7.08}$ $\rm 2.37^{--}_{--}$ $\rm 1.00^{--}_{--}$ 0.71 38
II+VI 0.582/0.680 $\rm0.31^{+0.04}_{-0.03}$ 0.59(fix) $\rm 1.43^{+0.20}_{-0.15}$ $\rm0.82^{+0.36}_{-0.25}$ 2.99(fix) $\rm 1.49^{+0.17}_{-0.20}$ 1.20 287
VII 0.765 $\rm0.49^{+0.08}_{-0.05}$ 0.59(fix) $\rm 1.92^{+0.40}_{-0.32}$ $\rm 1.47^{+0.75}_{-0.51}$ 2.99(fix) $\rm 1.53^{+0.31}_{-0.24}$ 1.05 126
III 0.828 $\rm0.71^{+0.11}_{-0.07}$ 0.59(fix) $\rm 2.34^{+1.17}_{-0.47}$ $\rm0.84^{+0.57}_{-0.26}$ 2.99(fix) $\rm 1.52^{+0.23}_{-0.26}$ 1.32 118
IV 0.903 $\rm 1.10^{+0.13}_{-0.13}$ 0.59(fix) $\rm 5.61^{+1.46}_{-0.93}$ $\rm 3.69^{+3.09}_{-1.84}$ 2.99(fix) $\rm 1.98^{+0.46}_{-0.55}$ 1.05 78
V 0.994 $\rm 1.68^{+0.26}_{-0.27}$ 0.59(fix) $\rm 6.99^{+2.46}_{-1.28}$ $\rm 7.36^{+6.56}_{-3.40}$ 2.99(fix) $\rm 2.53^{+1.87}_{-1.07}$ 0.74 40
II+VI 0.582/0.680 $\rm0.39^{+0.02}_{-0.02}$ 0.59(fix) 2.00(fix) $\rm 1.11^{+0.13}_{-0.12}$ 2.99(fix) 1.51(fix) 1.21 289
VII 0.765 $\rm0.51^{+0.03}_{-0.02}$ 0.59(fix) 2.00(fix) $\rm 1.50^{+0.25}_{-0.20}$ 2.99(fix) 1.51(fix) 1.03 128
III 0.828 $\rm0.68^{+0.08}_{-0.05}$ 0.59(fix) 2.00(fix) $\rm0.74^{+0.15}_{-0.14}$ 2.99(fix) 1.51(fix) 1.30 120
IV 0.903 $\rm0.80^{+0.09}_{-0.06}$ 0.59(fix) 2.00(fix) $\rm 1.03^{+0.21}_{-0.19}$ 2.99(fix) 1.51(fix) 1.09 80
V 0.994 $\rm 1.13^{+0.19}_{-0.12}$ 0.59(fix) 2.00(fix) $\rm 1.82^{+0.45}_{-0.35}$ 2.99(fix) 1.51(fix) 0.87 42

The first two columns specify the relevant spectrum. Columns 3-5 give respectively the absorbing column density, the plasma temperature and a normalisation factor (norm) equal to $\frac{10^{-14}}{4 \pi {d}^2} \int n_{\rm e} n_{\rm H} {\rm d}V$with d being the distance to the source (in cm), $n_{\rm e}$, $n_{\rm H}$the electron and hydrogen number densities respectively (in cm-3). The next three columns are dealing with the second component (power law); the seventh one gives the photon index whereas the eighth one gives the power-law normalisation. The last two columns give the reduced $\chi^2$ of the fit and the number of degrees of freedom. The quoted upper and lower values correspond to the 90% confidence interval (undetermined values are replaced by hyphens).

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