\begin{table}%t4
%\centering
\par
%\scriptsize
\caption{\label{tab:igrbfittotal}The same as Table~\ref{tab:igrbfit}, but for the spectrum of \igrB\ obtained by using the total available exposure time of the \XMM\ observation.}  
\begin{tabular}{@{}lccc@{}}
\noalign{\smallskip} 
\hline\hline
\noalign{\smallskip} 
Model & BB+CUTOFFPL & MKL+CUTOFFPL & BMC \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
$N_{\rm H}$ (10$^{22}$~cm$^{-2}$) & $\rm 0.9^{+0.2}_{-0.1}$ & $\rm 0.7^{+0.1}_{-0.2}$ & $\rm 1.0^{+0.1}_{-0.2}$ \\
\noalign{\smallskip}
$\Gamma$ & 1.6 $\pm$ 0.1 & 1.4 $\pm$ 0.1 & 2.0 $\pm$ 0.1 \\
\noalign{\smallskip}
$kT_{\rm BB}$ (keV) & $\rm 0.082^{+0.007}_{-0.004}$ & --- & --- \\
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$R_{\rm BB}$\tablefootmark{a} (km) & $\rm 100^{+126}_{-47}$ & --- & --- \\
\noalign{\smallskip}
$kT_{\rm MKL}$ (keV) & --- & $\rm 0.22^{+0.04}_{-0.02}$ & --- \\
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$N_{\rm MKL}$ (10$^{-3}$)  & --- & $\rm 1.3_{-0.8}^{+1.1}$ & --- \\
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$kT_{\rm BMC}$ (keV) & --- & --- & $\rm 0.075^{+0.007}_{-0.006}$ \\
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$\log(A)$       & --- & --- & $\rm --2.5^{+0.3}_{-0.2}$ \\
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$N_{\rm BMC}$ (10$^{-3}$) & ---  & --- & $\rm 2.0^{+2.8}_{-1.3}$ \\
\noalign{\smallskip} 
$F_{\rm 0.5{-}1.5~keV}$\tablefootmark{b} & $\rm 1.2_{-0.8}^{+0.1}$ & $\rm 1.2_{-0.7}^{+0.1}$ & $\rm 1.2_{-0.8}^{+0.2}$ \\
\noalign{\smallskip}
$F_{\rm 1.5{-}10~keV}$\tablefootmark{b} & $\rm 6.3_{-1.4}^{+0.7}$ & $\rm 6.3_{-1.0}^{+0.7}$ & $\rm 6.4_{-3.7}^{+0.9}$ \\
\noalign{\smallskip}
$F_{\rm 0.5{-}10~keV}$\tablefootmark{b} & $\rm 7.5_{-2.1}^{+0.6}$ & $\rm 7.5_{-1.5}^{+0.8}$ & $\rm 7.5_{-4.0}^{+1.1}$  \\
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$\chi^2_{\rm red}$/d.o.f.  & 0.99/99 & 1.05/99 & 1.02/99 \\
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EXP. (ks)\tablefootmark{c}  & 26 & 26 & 26 \\
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\hline
\noalign{\smallskip} 
\end{tabular}
\tablefoot{
\tablefoottext{a}{For a distance of 3~kpc.}
\tablefoottext{b}{Observed flux in units of 10$^{-13}$~erg~cm$^{-2}$~s$^{-1}$.} 
\tablefoottext{c}{Exposure time.}}
\end{table}