\begin{table}%T6
\caption{Fit results on the X-ray spectrum from \vinef\ (area~1).}
\label{tabgalfit}
%\centerline
 {
\begin{tabular}{llllllllll} 
\hline\hline
Model & $N_{\rm H}$ & $kT$ & $\Gamma$ & $Z$ & Norm & 
Red. $\chi^2$ & d.o.f. & $F_{\rm X}$ & $L_{\rm X}$\\
(1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) & (10)\\ 
[0.5mm]
\hline\\[-2.5mm]
RS & $\rm 0.50^{+0.16}_{-0.13}$ & $\rm 0.88^{+\infty}_{-0.04}$ & & 1 & 2.7 & 3.8 & 27 & 
$\rm 0.78^{+0.07}_{-0.78}$ & $\rm 0.74^{+0.07}_{-0.74}$ \\ [1mm]
RS & $\rm 2.26^{+0.26}_{-0.23}$ & $\rm 1.01^{+0.07}_{-0.08}$ & & 0.1 & 16 & 1.4 & 27 & 
1.31$\pm$0.01 & 1.24$\pm$0.01 \\ [1mm]
BS & $\rm 3.74^{+0.50}_{-0.45}$ & $\rm 0.74^{+0.11}_{-0.10}$ & & & 3.3 & 1.0 & 27 & 
$\rm 1.90^{+0.16}_{-0.14}$ & $\rm 1.80^{+0.15}_{-0.13}$ \\ [1mm]
PO & $\rm 6.01^{+0.78}_{-0.64}$ & & 2.81$\pm$0.17 & & 4.0 & 1.0 & 27 & $\rm 4.79^{+1.25}_{-0.94}$ & 
$\rm 4.54^{+1.18}_{-0.89}$ \\ [1mm]
RS + PO & $\rm 4.91^{+1.08}_{-0.92}$ & $\rm 0.57^{+0.25}_{-0.21}$ & $\rm 2.61^{+0.26}_{-0.16}$ & 
& 3.3 (PO) & 0.9 & 25 & $\rm 3.16^{+1.21}_{-0.52}$ & $\rm 3.00^{+1.15}_{-0.49}$ \\
 & & & & 1 & 0.38 (RS) & & & (0.15$\pm$0.03) & (0.14$\pm$0.03) \\ [1mm]
RS + PO & $\rm 4.77^{+0.96}_{-0.77}$ & $\rm 0.55^{+0.29}_{-0.21}$ & 2.56$\pm$0.37 & & 3.1 (PO) &
 0.9 & 25 & $\rm 2.95^{+1.62}_{-0.91}$ & $\rm 2.80^{+1.54}_{-0.86}$ \\
 & & & & 0.1 & 3.5 (RS) & & & $\rm (0.30^{+0.01}_{-0.07}$) & $\rm (0.28^{+0.01}_{-0.07}$) \\ [1mm]
RS + RS & $\rm 2.68^{+0.82}_{-0.72}$ & $\rm 4.34^{+\infty}_{-2.65}$ & & 1 & 6.8 & 1.1 & 25 & 
$\rm 1.50^{+0.42}_{-0.82}$ & $\rm 1.42^{+0.40}_{-0.78}$ \\
 & & $\rm 0.31^{+0.17}_{-0.08}$ & & 0.1 & 12 & & & $\rm (0.76^{+0.21}_{-0.08}$) 
& $\rm (0.72^{+0.20}_{-0.08}$) \\ 1mm]
RS + PO & 6.98 (PO, fixed) & $\rm 0.87^{+\infty}_{-0.86}$ & $\rm 3.12^{+0.47}_{-0.27}$ & & 2.9 (PO) & 
1.0 & 26 & $\rm 5.69^{+6.03}_{-2.04}$ & $\rm 5.39^{+5.71}_{-1.93}$ \\
 &  2.82 (RS, fixed) & & & 0.1 & 4.5 (RS) & & & $\rm (0.40^{+0.01}_{-0.39}$) 
& $\rm (0.38^{+0.01}_{-0.37}$) \\ [1mm]
\hline
\end{tabular}
}
\smallskip
Column (1): spectral models: BS = thermal Bremsstrahlung, RS = 
Raymond-Smith, PO = power law.\\ 
Column (2): column density in units of 10$^{20}$ cm$^{-2}$.\\ 
Column (3): plasma temperature in units of~keV.\\ 
Column (4): photon index.\\ 
Column (5): metallicity in units of $Z_{\odot}$; fixed values.\\
Column (6): scaling factor: for BS in units of 
(10$^{-18}$/(4$\pi D^2$))$\int n_{\rm e}n_{\rm I}$d$V$, 
$n_{\rm e}, n_{\rm I}$ = electron and ion densities 
(cm$^{-3}$); for RS in units of 
(10$^{-18}$/(4$\pi D^2$))$\int n_{\rm e}^2$d$V$, 
$n_{\rm e}, n_{\rm H}$ = electron and \HI\ density
(cm$^{-3}$); for PO in units of 10$^{-4}$ photons~keV$^{-1}$ 
cm$^{-2}$ s$^{-1}$ at 1~keV.\\ 
Column (7): reduced $\chi^2$.\\ 
Column (8): degrees of freedom.\\ 
Column (9): unabsorbed X-ray flux in units of 10$^{-12}$ erg cm$^{-2}$ s$^{-1}$. 
Values in brackets give the contribution of the thermal component.\\ 
Column (10): X-ray luminosity in units of 10$^{40}$ erg s$^{-1}$. 
Values in brackets give the contribution of the thermal component. For the RS+RS model the values 
in brackets are for the low-temperature component.
\end{table}