\begin{table}%T2
\caption{Observed and emitted fluxes  
of SN~2002ap on 2002 February 2, for three different spectral models 
consistent with the observed X-ray count rates in the EPIC pn and MOS 
bands (Table~\ref{tab1}). A distance of 7.3~Mpc has been assumed. 
Fluxes are in units of $10^{-15}$~erg~cm$^{-2}$ s$^{-1}$.} 
%Luminosities are in units of $10^{37}$\lum. }
\label{tab2} 
%\centering
\par
         \begin{tabular}[width=textwidth]{lcccc}
            \hline
            \hline
            \noalign{\smallskip}
	Instrument & Flux & Flux  & Flux & Flux \\
        & ($0.3$--$12.0$)~keV & ($0.3$--$1$)~keV & ($1$--$2$)~keV & ($2$--$12$)~keV\\
            \noalign{\smallskip}
            \hline\\
& \multicolumn{4}{c}{model: $n_{\rm H} = 5 \times 10^{21}$~cm$^{-2}$; 
 $kT_{\rm {rs}} = 0.50$~keV; $Z=Z_{\odot}$}\\[5pt]  
\hline \\
            \noalign{\smallskip} 
pn observed flux & $4.9\pm0.6$ & $2.8\pm0.4$ & $1.9\pm0.4$ & $0.2\pm1.2$ \\
MOS1 observed flux & $4.0\pm1.0$  & & & \\
MOS2 observed flux & $4.1\pm1.0$  & & & \\[5pt]
pn emitted flux & $25.7\pm3.1$ & $21.5\pm2.9$ & $3.9\pm0.8$ & $0.2\pm1.2$ \\
MOS1 emitted flux & $21.1\pm5.1$  & & & \\
MOS2 emitted flux & $21.4\pm5.2$  & & & \\[5pt]
%pn emitted luminosity & $16.4\pm2.0$ & $13.7\pm1.9$ & $2.5\pm0.5$ & $0.1\pm0.8$ \\
%MOS1 emitted luminosity & $13.4\pm3.2$  & & & \\
%MOS2 emitted luminosity & $13.7\pm3.3$  & & & \\[5pt]
  \noalign{\smallskip}
            \hline \\
& \multicolumn{4}{c}{model: $n_{\rm H} = 3 \times 10^{21}$~cm$^{-2}$; 
 $kT_{\rm {rs}} = 0.75$~keV; $Z=Z_{\odot}$}\\[5pt]  
\hline \\
            \noalign{\smallskip} 
pn observed flux & $5.2\pm0.6$ & $2.9\pm0.4$ & $2.0\pm0.4$ & $0.2\pm1.2$ \\
MOS1 observed flux & $4.1\pm1.1$  & & & \\
MOS2 observed flux & $4.2\pm1.1$  & & & \\[5pt]
pn emitted flux & $12.4\pm1.5$ & $9.2\pm1.2$ & $3.1\pm0.7$ & $0.2\pm1.2$ \\
MOS1 emitted flux & $9.9\pm2.4$  & & & \\
MOS2 emitted flux & $10.0\pm2.4$  & & & \\[5pt]
%pn emitted luminosity & $7.9\pm1.0$ & $5.9\pm0.8$ & $2.0\pm0.4$ & $0.1\pm0.8$ \\
%MOS1 emitted luminosity & $6.3\pm1.5$  & & & \\
%MOS2 emitted luminosity & $6.4\pm1.5$  & & & \\[5pt]
  \noalign{\smallskip}
            \hline \\
& \multicolumn{4}{c}{model: $n_{\rm H} = 0.5 \times 10^{21}$~cm$^{-2}$; 
 $kT_{\rm {rs}} = 0.85$~keV; $Z=Z_{\odot}$}\\[5pt]  
\hline \\
            \noalign{\smallskip} 
pn observed flux & $5.0\pm0.6$ & $2.8\pm0.4$ & $2.0\pm0.4$ & $0.2\pm1.2$ \\
MOS1 observed flux & $4.1\pm1.1$  & & & \\
MOS2 observed flux & $4.2\pm1.1$  & & & \\[5pt]
pn emitted flux & $5.9\pm0.7$ & $3.6\pm0.5$ & $2.0\pm0.4$ & $0.2\pm1.2$ \\
MOS1 emitted flux & $4.9\pm1.3$  & & & \\
MOS2 emitted flux & $5.0\pm1.3$  & & & \\[5pt]
%pn emitted luminosity & $3.8\pm0.5$ & $2.3\pm0.3$ & $1.3\pm0.3$ & $0.1\pm0.8$ \\
%MOS1 emitted luminosity & $3.1\pm0.8$  & & & \\
%MOS2 emitted luminosity & $3.2\pm0.8$  & & & \\[5pt]
\hline
	\end{tabular}
   \end{table}