\begin{table}%T4
  \caption{\label{TabFitParams}Table of fit parameters for the phase-averaged broad band
             spectrum shown in Fig.~\ref{FigBbSpectrum} for two
             different spectral models (see text). A systematic
             error of 2\% was assumed. The uncertainties given are
             at 90\% confidence level for single parameter errors
             ($\chi^2_{\rm min} + 2.7$).}
  \small%\centerline
{
  \begin{tabular}{l l l c c c c c c c}
    \hline \hline\noalign{\smallskip}
           Compon. & Parameter                      & Unit                           & Model A               & Model B               & Ref.$^a$ & Ref.$^b$      & Ref.$^c$ & Ref.$^d$ & Ref.$^e$\\
    \hline\noalign{\smallskip}
           phabs   & $N_{\rm H}$ (JEM-X1, ISGRI) & $10^{22}$ cm$^{-2}$            &                       &   $0$ (frozen)        &   1.29 &  14.1        & 41    & 12.7 &  7.2 \\
           phabs   & $N_{\rm H}$ (JEM-X2)        & $10^{22}$ cm$^{-2}$            &                       &   $\rm 18.4^{+3.7}_{-3.6}$&        &              &       &      &      \\
           powerlaw  & $\Gamma$ (JEM-X2, ISGRI)     &                                &   $1$ (frozen)        &   $1.27 \pm 0.05$    &   1.07 &              & 1.0   & 0.83 &  0.60 \\
           powerlaw  & $\Gamma$ (JEM-X1)            &                                &   $1.3$ (frozen)      &   $1.27\pm 0.05$    &        &              &       &      &   \\
           powerlaw  & normalisation (1~keV)        & (keV cm$^{2}$ s)$^{-1}$   &  $\rm 0.055^{+0.003}_{-0.002}$ &   $0.12 \pm 0.02 $    &   0.06 &              & 0.046 &      &   \\
           highecut  & Cutoff energy                & keV                            &  $\rm 21.6^{+1.0}_{-1.4}$ &  $24.4 \pm 0.9 $      &  12.82 &              &       & 13.0 &  $<$5.0 \\
           highecut  & Folding energy               & keV                            &  $19.0 \pm 0.2 $      &  $21.2\pm 0.5$      &  29.37 &              &       & 21.2 &   17.0 \\
           Gaussian  & Fe line centre               & keV                            &                       &                       &   6.65 &  6.4/7.1   & 6.4   & 6.47 &   6.60 \\
           Gaussian  & Fe line width $(\sigma)$     & keV                            &                       &                       &   0.40 &  0.2/0.3   & 0.044 & 0.42 &   0.24 \\
           Gaussian  & Total flux in Fe line        & $10^{-3}$ (cm$^{2}$ s)$^{-1}$  &                       &                       &   2.77 &  0.74/0.25 & 0.8   &      &   3.0 \\
    \hline
           energy range  &                          & keV                            & 6--160                & 6--160                &  3--100 & 0.5--10      & 4--8 & 1--100 & 3--40 \\
           red.~$\chi^2$ &                          &                                & 1.00                  & 0.94                         \\
           d.o.f.           &                          &                                & 258                   & 253                          \\
    \hline
  \end{tabular}
  }
  \smallskip
    $^{{a}}$ \citet{Baykal2000};
    $^{{b}}$ \citet{Audley2006}, non eclipse spectrum, 2 Fe lines;
    $^{{c}}$ \citet{2002ApJ...573..789C};
    $^{{d}}$ \citet{Orland1999};
    $^{{e}}$ \citet{1990PASJ...42..785K}.
\end{table}