\begin{table}%t5
\par
\caption {\label{tab5}Results of the fit to the individual X-ray
spectra of models of the kind 
{\tt{wabs1$\ast$mekal+wabs2$\ast$powerlaw}}. } 
%\centerline
 {\begin{tabular}{lccccccccc}
\hline\hline \\[-8pt]
No. & Phase & $N_{{\rm H1}}$ & $kT_1$ & Norm$_1$ & $N_{{\rm H2}}$ & 
Ph.I. & Norm$_2$ & $\chi_{\nu}^{2}$ & d.o.f. \\  
&& (10$^{22}$~cm$^{-2}$) & (keV) & (10$^{-4}$~cm$^{-5}$) &
(10$^{22}$~cm$^{-2}$) && (10$^{-4}$~cm$^{-5}$) 
&& \\
\hline \\[-8pt]
II+VI & 0.582/0.680 & $\rm 0.37^{+0.11}_{-0.16}$ & $\rm 0.59^{+0.03}_{-0.03}$ &
$\rm 1.51^{+0.57}_{-0.46}$ & $\rm 0.30^{+0.40}_{-0.15}$ & $\rm 2.47^{+0.42}_{-0.18}$ &
$\rm 0.76^{+0.49}_{-0.26}$ & 1.20 & 285 \\[1pt]
VII & 0.765 & $\rm 0.50^{+0.08}_{-0.20}$ & $\rm 0.60^{+0.04}_{-0.04}$ &
$\rm 1.93^{+0.42}_{-0.90}$ & $\rm 1.28^{+1.30}_{-0.89}$ & $\rm 3.01^{+0.36}_{-0.66}$ &
$\rm 1.57^{+3.23}_{-0.77}$ & 1.07 & 124 \\[1pt]
III & 0.828 & $\rm 0.67^{+0.14}_{-0.14}$ & $\rm 0.58^{+0.05}_{-0.05}$ &
$\rm 2.15^{+1.25}_{-1.01}$ & $\rm 0.74^{+0.69}_{-0.60}$ & $\rm 3.21^{+0.24}_{-0.72}$ &
$\rm 2.01^{+1.25}_{-1.27}$ & 1.34 & 116 \\[1pt]
IV & 0.903 & $\rm 1.11^{+0.06}_{-0.30}$ & $\rm 0.61^{+0.07}_{-0.06}$ &
$\rm 5.72^{+1.98}_{-2.95}$ & $\rm 4.16^{+9.83}_{-4.53}$ & $\rm 3.01^{+2.76}_{-2.31}$ &
$\rm 2.13^{--}_{--}$ & 1.08 & 76 \\[1pt]
V & 0.994 & $\rm 1.58^{+0.26}_{-0.26}$ & $\rm 0.71^{+0.19}_{-0.12}$ &
$\rm 5.01^{+2.57}_{-2.03}$ & $\rm 7.08^{+7.17}_{-7.08}$ & $\rm 2.37^{--}_{--}$ &
$\rm 1.00^{--}_{--}$ & 0.71 & 38 \\
\smallskip \\
II+VI & 0.582/0.680 & $\rm 0.31^{+0.04}_{-0.03}$ & 0.59(fix) &
$\rm 1.43^{+0.20}_{-0.15}$ & $\rm 0.82^{+0.36}_{-0.25}$ & 2.99(fix) &
$\rm 1.49^{+0.17}_{-0.20}$ & 1.20 & 287 \\[1pt]
VII & 0.765 & $\rm 0.49^{+0.08}_{-0.05}$ & 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 \\[1pt]
III & 0.828 & $\rm 0.71^{+0.11}_{-0.07}$ & 0.59(fix) &
$\rm 2.34^{+1.17}_{-0.47}$ & $\rm 0.84^{+0.57}_{-0.26}$ & 2.99(fix) &
$\rm 1.52^{+0.23}_{-0.26}$ & 1.32 & 118 \\[1pt]
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 \\[1pt]
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 \\
\smallskip \\
II+VI & 0.582/0.680 & $\rm 0.39^{+0.02}_{-0.02}$ & 0.59(fix) &
2.00(fix) & $\rm 1.11^{+0.13}_{-0.12}$ & 2.99(fix) &
1.51(fix) & 1.21 & 289 \\[1pt]
VII & 0.765 & $\rm 0.51^{+0.03}_{-0.02}$ & 0.59(fix) &
2.00(fix) & $\rm 1.50^{+0.25}_{-0.20}$ & 2.99(fix) &
1.51(fix) & 1.03 & 128 \\[1pt]
III & 0.828 & $\rm 0.68^{+0.08}_{-0.05}$ & 0.59(fix) &
2.00(fix) & $\rm 0.74^{+0.15}_{-0.14}$ & 2.99(fix) &
1.51(fix) & 1.30 & 120 \\[1pt]
IV & 0.903 & $\rm 0.80^{+0.09}_{-0.06}$ & 0.59(fix) &
2.00(fix) & $\rm 1.03^{+0.21}_{-0.19}$ & 2.99(fix) &
1.51(fix) & 1.09 & 80 \\[1pt]
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 \\[1pt]
\hline
\end{tabular}}
\smallskip
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).
\end{table}