\begin{table}%t3
%\centering
\par
%\scriptsize
\caption{\label{tab:igrbfit}The same as Table~\ref{tab:xtefit}, but for the time-resolved spectra of \igrB.}  
\begin{tabular}{@{}lccccccccc@{}}
\hline\hline
\noalign{\smallskip} 
Model & \multicolumn{3}{c}{BB+CUTOFFPL} & \multicolumn{3}{c}{MKL+CUTOFFPL} & \multicolumn{3}{c}{BMC} \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
& $<$0.1 & 0.1--0.2 & $>$0.2 & $<$0.1 & 0.1--0.2 & $>$0.2 & $<$0.1 & 0.1--0.2 & $>$0.2 \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
$N_{\rm H}$ (10$^{22}$~cm$^{-2}$) & $\rm 1.0^{+0.4}_{-0.3}$ & $\rm 0.8^{+0.2}_{-0.3}$ & 1.2 $\pm$ 0.3 & $\rm 0.7^{+0.1}_{-0.4}$ & 0.6 $\pm$ 0.2 & $\rm 0.9^{+0.2}_{-0.3}$ & 1.1 $\pm$ 0.3 & $\rm 0.9^{+0.2}_{-0.3}$ & 1.4 $\pm$ 0.3 \\
\noalign{\smallskip}
$\Gamma$ & $\rm 2.1^{+0.4}_{-0.3}$ & 1.7 $\pm$ 0.2 & 1.3 $\pm$ 0.2 & 1.7 $\pm$ 0.2 & $\rm 1.6^{+0.1}_{-0.2}$ & $\rm 1.1^{+0.1}_{-0.2}$ & $\rm 2.6^{+0.3}_{-0.2}$ & $\rm 2.1^{+0.2}_{-0.1}$ & 1.7 $\pm$ 0.2 \\
\noalign{\smallskip}
$kT_{\rm BB}$ (keV) & 0.08 $\pm$ 0.02 & $\rm 0.08^{+0.02}_{-0.01}$ & $\rm 0.08^{+0.01}_{-0.02}$ & --- & --- & --- & --- & --- & --- \\
\noalign{\smallskip}
$R_{\rm BB}^{a}$ (km) & $\rm 156_{-46}^{+733}$ & $\rm 82_{-60}^{+160}$ & $\rm 286_{-224}^{+795}$ & --- & --- & --- & --- & --- & --- \\
\noalign{\smallskip}
$kT_{\rm MKL}$ (keV) & --- & --- & --- & $\rm 0.22^{+0.14}_{-0.04}$ & $\rm 0.21^{+0.07}_{-0.04}$ & $\rm 0.20^{+0.10}_{-0.04}$ & --- & --- & --- \\
\noalign{\smallskip}
$N_{\rm MKL}$ (10$^{-3}$)  & --- & --- & --- & $\rm 1.0_{-0.7}^{+2.0}$ & $\rm 1.1_{-1.0}^{+3.6}$ & $\rm 7.7_{-6.8}^{+74.0}$ & --- & --- & --- \\
\noalign{\smallskip}
$kT_{\rm BMC}$ (keV) & --- & --- & --- & --- & --- & --- & 0.07 $\pm$ 0.01 & 0.08 $\pm$ 0.01 & 0.07 $\pm$ 0.01 \\
\noalign{\smallskip}
$\log(A)$       & --- & --- & --- & --- & --- & --- & $\rm --2.8^{+0.5}_{-0.2}$ & $\rm --2.1^{+0.4}_{-0.3}$ & $\rm --2.9^{+0.7}_{-0.5}$ \\
\noalign{\smallskip} 
$N_{\rm BMC}$ (10$^{-3}$) & ---  & --- & --- & --- & --- & --- & $\rm 4.3^{+22.3}_{-3.7}$ & $\rm 1.1^{+2.5}_{-1.1}$ & $\rm 16.4^{+75.5}_{-14.4}$ \\
\noalign{\smallskip} 
$F_{\rm 0.5-1.5~keV}^{b}$ & $\rm 0.84_{-0.76}^{+0.05}$ & $\rm 1.4_{-1.0}^{+0.1}$ & $\rm 3.0_{-2.1}^{+0.2}$ & $\rm 0.84_{-0.64}^{+0.12}$ & $\rm 1.4_{-0.9}^{+0.2}$ & $\rm 3.0_{-1.8}^{+0.1}$ & $\rm 0.83_{-0.83}^{+0.12}$ & $\rm 1.4_{-1.4}^{+0.3}$ & $\rm 2.9_{-2.0}^{+0.2}$ \\
\noalign{\smallskip}
$F_{\rm 1.5-10~keV}^{b}$ & $\rm 2.2_{-1.3}^{+0.4}$ & $\rm 6.2_{-2.8}^{+1.1}$ & $\rm 38.1_{-12.0}^{+6.0}$ & $\rm 2.3_{-0.8}^{+0.5}$ & $\rm 6.3_{-2.1}^{+1.0}$ & $\rm 38.5_{-10.1}^{+5.5}$ & $\rm 2.2_{-1.3}^{+0.4}$ & $\rm 6.2_{-6.2}^{+1.4}$ & $\rm 38.6_{-32.6}^{+1.1}$ \\
\noalign{\smallskip}
$F_{\rm 0.5-10~keV}^{b}$ & $\rm 3.0_{-1.9}^{+0.4}$ & $\rm 7.6_{-3.3}^{+1.0}$ & $\rm 41.1_{-17.0}^{+5.0}$ & $\rm 3.2_{-1.5}^{+0.4}$ & $\rm 7.7_{-3.2}^{+1.2}$ & $\rm 41.5_{-12.0}^{+5.0}$ & $\rm 2.9_{-2.7}^{+0.4}$ & $\rm 7.7_{-7.7}^{+1.3}$ & $\rm 41.5_{-29.8}^{+1.1}$ \\
\noalign{\smallskip}
$\chi^2_{\rm red}$/d.o.f.  & 0.8/26 & 1.2/42 & 0.7/38 & 0.8/26 & 1.2/42 & 0.8/38 & 0.8/26 & 1.2/42 & 0.7/38 \\
\noalign{\smallskip}
EXP. (ks)\tablefootmark{c}  & 13 & 9 & 2 & 13 & 9 & 2 & 13 & 9 & 2  \\
%\noalign{\smallskip}
\hline
\end{tabular}
\tablefoot{In all cases, the cutoff energy is fixed at 11~keV (see Sect.~\ref{sec:igrresults}). For the BMC model, we reported 
below the value $\Gamma=\alpha+1$, where $\alpha$ is the Comptonization efficiency of the model, the value of the 
``illumination parameter'' $\log(A)$, and the normalization $N_{\rm BMC}$.
\tablefoottext{a}{For a distance of 3~kpc.}
\tablefoottext{b}{Observed flux in unit of 10$^{-13}$~erg~cm$^{-2}$~s$^{-1}$.}
\tablefoottext{c}{Exposure time.}}
\end{table}