\begin{table}%ta6
\caption{(\emph{Left}) Additional fit results for Cen~A (3EG~J$1324-4314$) with the model composed of an absorbed power law, plus one or two
Gaussian emission lines. Fit performed in the $4{-}10$~keV energy band and then extrapolated to $0.4{-}10$~keV. 
The two columns refer to the two observations. The rows list the following parameters:
(1) absorbing column density [$10^{20}$~cm$^{-2}$];
(2) photon index of the power law model;
(3)~normalization of the power law model [$10^{-2}$~ph~cm$^{-2}$~s$^{-1}$~keV$^{-1}$ at $1$~keV]; 
(4) energy of the emission line 1~[keV];
(5) line width $\sigma$ 1~[keV];
(6) flux of the emission line 1 [$10^{-4}$~ph~cm$^{-2}$~s$^{-1}$];
(7) equivalent width of the emission line 1 [eV];
(8) energy of the emission line 2~[keV];
(9)~line width $\sigma$ 2~[keV];
(10) flux of the emission line 2 [$10^{-4}$~ph~cm$^{-2}$~s$^{-1}$];
(11) equivalent width of the emission line 2 [eV];
(12) reduced $\chi^2$ and degrees of freedom;
(13) observed flux in the $0.4{-}10$~keV energy band [$10^{-11}$~erg~cm$^{-2}$~s$^{-1}$];
(14) intrinsic luminosity in the $0.4{-}10$~keV energy band rest frame [$10^{45}$~erg~s$^{-1}$].
The uncertainties in the parameter estimates are at the $90\%$ confidence limit for one parameter of interest. 
For $N_{{\rm H}}={\rm Gal}$, it means that the absorption column has been fixed to the 
Galactic value. The luminosities were calculated using $d=3.84$~Mpc. 
(\emph{Right}) EPIC~spectrum in the $4{-}10$~keV energy band.}\label{tab:srcdata4}
%\centering
\par
%\begin{minipage}{5.5cm}
\small\begin{tabular}{lcc}
\hline\hline
{} & $0093650201$ & $0093650301$ \\
\hline\noalign{\smallskip}
$N_{{\rm H}}$ & $\rm 1420_{-90}^{+40}$     & $1800\pm 200$\\
$\Gamma$         & $\rm 2.24_{-0.04}^{+0.07}$ & $2.3\pm 0.2$\\
$A_{\rm pl}$     & $\rm 22.1_{-1.2}^{+0.3}$   & $\rm 32_{-10}^{+13}$\\
$E_1$            & $6.41\pm 0.02$         & $6.44\pm 0.02$\\
$\sigma_1$       & $<$$0.074$               & $<$$0.065$ \\
$A_{\rm L1}$     & $\rm 2.6_{-0.6}^{+0.8}$    & $\rm 4.6_{-1.0}^{+1.1}$ \\
$EqW_1$          & $\rm 70_{-16}^{+22}$       & $\rm 107_{-23}^{+26}$\\
$E_2$            & $\rm 6.8_{-0.4}^{+0.3}$    & --\\
$\sigma_2$       & $\rm 0.76_{-0.25}^{+0.39}$ & --\\
$A_{\rm L2}$     & $\rm 4.3_{-2.3}^{+4.4}$    & --\\
$EqW_2$          & $\rm 133_{-71}^{+135}$     & --\\
$\tilde{\chi}^2$/d.o.f. &  $0.99/984$        & $0.96/498$\\
$F$              &  $17.4$                & $18.5$\\
$L$              &  $3.1\times 10^{-4}$  & $3.3\times 10^{-4}$\\
\hline
\end{tabular}
%\end{minipage}
\hspace*{10mm}
%\begin{minipage}{9.3cm}
\includegraphics[scale=0.4,angle=270]{4921_tA6.ps}
%\end{minipage}
\end{table}