\begin{table}%t2
\caption{Results from absorbed power-law fits to the EPIC spectra.}
%\centerline
{\begin{tabular}{lcccccc}
\hline\hline\noalign{\smallskip}
 Date                    & 2000-10-17    & 2001-11-21           & 2005-11-27          & 2005-11-29	    & 2005-12-11 	 & 2005 combined       \\
 Modified Julian Day     & 51834.75      & 52234.16             & 53701.37            & 53703.32            & 53715.66           & $-$                 \\
 Orbital phase$^1$       & 0.17          & 0.31                 & 0.84                & 0.85                & 0.95               & $-$                 \\
 SMC \nh\ (\ohcm{20})    & $<$6.2        &     $-$              & $\rm 3.9_{-3.7}^{+3.9}$ & $\rm 4.8_{-4.4}^{+4.9}$ & $\rm 3.0_{-3.0}^{+15}$ & $\rm 3.7_{-2.1}^{+2.3}$ \\ 
 Photon index            & $0.76\pm0.08$ &     $-$              & $0.68\pm0.04$       & 0.72$\pm$0.05	    & $0.75\pm0.11$	 & 0.70$\pm$0.02       \\
 $\chi^2_r$/degrees of freedom & 0.99/43 &     $-$              & 1.37/127            & 1.07/120            & 0.97/29            & 1.23/280            \\
 Flux (\oergcm{-12})$^2$ & 1.3 (M2)	 &     $-$              & 5.9 (M1)            & 5.5 (M1) 	    & 2.2 (M1)		 &      $-$            \\
 Luminosity (\oergs{36}) & 0.57		 & $<2.8\times 10^{-3}$ & 2.6                 & 2.4		    & 0.96		 &      $-$            \\
\hline
\end{tabular}}\medskip
\par
$^1$ Using an orbital period of 127.3 days and the ephemeris for maximum optical light of MJD 52194.7 \citep{2006AJ....132..971S} as phase 0.
\\
$^2$ X-ray fluxes and luminosities are given for energies 0.2--10.0~keV and the instrument from which they were 
derived is indicated: EPIC-MOS1 (M1); EPIC-MOS2 (M2). Errors denote the 90\% confidence level. 
\label{tab-fits}
\end{table}