\begin{table}%t1
  \caption {\label{tab:param}Best fit parameters obtained from modeling the joint XIS
      and HXD data in the 5--60~keV band.}
%\centerline
 {\begin{tabular}{llll}
\hline\hline\rule{0mm}{3.5mm}
$A_{{\rm cutoffpl}}=3.79_{-0.03}^{+0.05}\times 10^{-2}$ &
$F_{{\rm Fe\ K}\alpha_1}=3.7\pm0.1\times 10^{-3}$  &
$F_{{\rm Fe\ K}\alpha_2}=1.85\pm0.05\times 10^{-3}$ \\
&
$F_{{\rm Fe\ K}\beta_1}=3.2_{-0.4}^{+0.3}\times 10^{-4}$ &
$F_{{\rm Fe\ K}\beta_3}=1.57_{-0.20}^{+0.15}\times 10^{-4}$ &
$F_{{\rm Ni\ K}\alpha}=7.4_{-2.7}^{+2.2}\times 10^{-4}$ \\[1mm]
\hline\rule{0mm}{3.5mm}
$c=1.00\pm0.01$ & 
$\Gamma=0.676_{-0.042}^{+0.009}$ &
$E_{\rm Fold} =20.5_{-0.3}^{+0.6}$~keV \\[1mm]
$N_{\rm H}=1.95_{-0.03}^{+0.02}\times  10^{24}~{\rm cm}^{-2}$ &
$A_{\rm Fe} =1.14_{-0.02}^{+0.03}$ \\[1mm]
$E_{{\rm Fe\ K}\alpha_1}=6404_{-2}^{+3}$~eV& 
${\it EW}_{{\rm Fe\ K}\alpha_1}=467_{-54}^{+13}$~eV&
$E_{{\rm Fe\ K}\alpha_2}=6391_{-2}^{+3}$~eV& 
${\it EW}_{{\rm Fe\ K}\alpha_2}=233_{-27}^{+7}$~eV\\[1mm]
$E_{{\rm Fe\ K}\beta_1}=7093_{-14}^{+13}$~eV &
${\it EW}_{{\rm Fe\ K}\beta_1}=44.1_{-5.2}^{+1.4}$~eV &
$E_{{\rm Fe\ K}\beta_3}=7092_{-14}^{+13}$~eV &
${\it EW}_{{\rm Fe\ K}\beta_3}=22.1_{-2.7}^{+0.6}$~eV \\[1mm]
$E_{{\rm Ni\ K}\alpha}=7446_{-51}^{+46}$~eV& 
${\it EW}_{{\rm Ni\ K}\alpha}=108_{-12.7}^{+4}$~eV\\[1mm]
\hline\rule{0mm}{3.5mm}
$F_{5.0-60~{\rm keV}}^{\rm ~absorbed}=3.4_{-0.1}^{+0.7}~10^{-10}~{\rm erg}~{\rm cm}^{-2}~{\rm s}^{-1}$ &
$F_{5.0-60~{\rm keV}}^{\rm ~unabsorbed}=2.43_{-0.09}^{+0.44}~10^{-9}~{\rm erg}~{\rm cm}^{-2}~{\rm s}^{-1}$ &
$\chi^2/{\rm d.o.f.}=242.6/245$ &
$\chi^2_{\rm red}=0.99$ \\[1mm]
\hline
\end{tabular}}
\par
\smallskip
 {We list the photon
      index ($\Gamma$), folding energy ($E_{\rm Fold}$), hydrogen equivalent
      column ($N_{\rm H}$), Fe abundance ($A_{\rm Fe}$), the
      total absorbed and unabsorbed fluxes, and the energy~($E$) and
      equivalent width (${\it EW}$) of the fluorescence lines. The norm
      of the absorbed cutoff powerlaw ($A_{{\rm cutoffpl}}$) is
      defined as the photon flux at 1~keV; for the absorbed Gaussian
      lines the norm~($F$) equals the total line flux.}
\end{table}