\begin{table}%t2
\caption{Spectral parameters inferred from  data from XMM1 and XMM2.\label{spec}}
\small%\centerline
{
\begin{tabular}{llllllllll}
\hline\hline\noalign{\smallskip}
Parameter & BB  & BB+BB & BB+BB$^{a}$  & PL & BB+PL  & BB+PL$^{b}$  & BB+PL$^{c}$  & BKPL & BREMSS\\
\noalign{\smallskip}\hline\noalign{\smallskip}
	  $N_{\rm H}$($10^{21}\mbox{cm}^{-2}$) & $\rm 2.67^{+0.09}_{-0.09}$ & $\rm 4.54^{+0.49}_{-0.43}$ & $\rm 6.38^{+0.21}_{-0.13}$ & $\rm 9.26^{+0.14}_{-0.17}$ & $\rm 8.57^{+0.88}_{-0.35}$ & $4.00$ & 8.02 & $\rm 7.62^{+0.17}_{-0.36}$ & $\rm 5.76^{+0.11}_{-0.11}$ \\\noalign{\smallskip}
	  $\Gamma_{1}$                     & --& -- & -- & $\rm 4.29^{+0.02}_{-0.02}$ & $\rm 4.67^{+0.14}_{-0.05}$ & $\rm 2.51^{+0.11}_{-0.13}$ & 3.50 & $\rm 3.61^{+0.05}_{-0.05}$ & --\\\noalign{\smallskip}
	  $\Gamma_{2}$                     & -- & -- & -- & -- & -- & -- & -- & $\rm 5.29^{+0.20}_{-0.18}$ & --\\\noalign{\smallskip}
	  $T_{1}$ ($10^{6}$~K)              & $\rm 4.32^{+0.04}_{-0.03}$ & $\rm 2.61^{+0.30}_{-0.26}$ & $\rm 1.87^{+0.02}_{-0.02}$ & -- & $\rm 4.43^{+0.05}_{-0.07}$ & $\rm 3.80^{+0.06}_{-0.05}$ & 1.87 & - & $\rm 9.57^{+0.18}_{-0.06}$\\\noalign{\smallskip}
	  $T_{2}$ ($10^{6}$~K)              & -- & $\rm 5.04^{+0.28}_{-0.20}$ & $\rm 4.58^{+0.03}_{-0.07}$ & -- & -- & -- & -- & -- & --\\\noalign{\smallskip}
	  $R_{1}$ (km)                     & $\rm 1.23^{+0.03}_{-0.02}$ & $\rm 3.29^{+1.12}_{-0.74}$ & 10 & -- & $\rm 0.89^{+0.06}_{-0.08}$ & $\rm 1.59^{+0.06}_{-0.06}$ & 10 & -- & --\\\noalign{\smallskip}
	  $R_{2}$ (km)                     & -- & $\rm 0.75^{+0.12}_{-0.15}$ & $\rm 1.09^{+0.04}_{-0.04}$ & -- & -- & -- & -- & -- & --\\\noalign{\smallskip}
	  $N_{\mbox{bremss}}$ ($10^{-2}$ cm$^{-5}$)  & -- & -- & -- & -- & -- & -- & -- & -- & $\rm 1.28^{+0.02}_{-0.02}$\\\noalign{\smallskip}
	  $F_{X_{0.1{-}2.4~{\rm keV}}}$ (erg  cm$^{-2}$ s$^{-1}$) & $5.82\times10^{-12}$ & $9.67\times10^{-12}$ & $2.04\times10^{-11}$ & $1.77\times10^{-9}$ & $2.60\times10^{-9}$ & $1.18\times10^{-11}$ & $2.18\times10^{-10}$ & $3.45\times10^{-10}$ & $2.40\times10^{-11}$\\\noalign{\smallskip}
	  $F_{X_{0.5{-}10~{\rm keV}}}$ (erg  cm$^{-2}$ s$^{-1}$) & $6.05\times10^{-12}$ & $8.94\times10^{-12}$ & $1.48\times10^{-11}$ & $4.46\times10^{-11}$ & $3.88\times10^{-11}$ & $8.28\times10^{-12}$ & $2.69\times10^{-11}$ & $2.48\times10^{-11}$ & $1.27\times10^{-11}$\\\noalign{\smallskip}
	  Reduced $\chi^{2}$              & 1.82 & 1.20 & 1.28 & 1.91  & 1.21 & 1.42 & 3.77 & 1.22 & 1.20\\\noalign{\smallskip}
	  d.o.f.                          & 467  & 465  & 466 & 467 & 465 & 466 & 467 & 465 & 467\\
\hline
\end{tabular}}
\smallskip
The emitting areas inferred from the blackbody fits are calculated for the assumed distance of 2.2 kpc.\\ 
$F_{X_{0.1{-}2.4~{\rm keV}}}$ and $F_{X_{0.5{-}10~{\rm keV}}}$ are unabsorbed fluxes in the energy range $0.1{-}2.4$~keV and $0.5{-}10$~keV, respectively.\\
$^{{a}}$ $R_{1}$ fixed at 10~km radius.\\
$^{{b}}$ $N_{\rm H}$ fixed at $4\times10^{21}\mbox{cm}^{-2}$.\\
$^{{c}}$ $R_{1}$ and $T_{1}$ fixed at 10 km and $1.87\times10^{6}$ K respectively.
 \end{table}