\begin{table}%t4
\caption{\label{burstTable}Burst parameters.} 
%\centerline
 {\tiny 
\begin{tabular}{lccccccccccc}
\hline \hline\noalign{\smallskip}
Id.$^a$
& Burst Start Time 
& $kT_{\rm peak}$$^b$ 
& $R_{\rm peak}$$^c$ 
& $\chi^2/$d.o.f. 
& $F_{\rm peak}$$^d$ 
& $f_{\rm b}$$^e$
& $\tau_{\rm fit}$$^f$
& $\tau_{\rm calc}$$^g$ 
& $F_{\rm pers}$$^h$
& $\Delta t$$^i$
& $\gamma$$^j$\\
~ & [UTC] & [keV] & [km] & ~ & ~ & ~ & [s] & [s] &~ & [s] & [$10^{-3}$] \\
\hline
1~~~~JEM-X  & 2005 Mar. 24,  14:26:23	& $2.3^{\rm +0.8}_{-0.5}$ & $7^{\rm +5}_{-3}$ 	& 15.7/12 		& $3.2^{\rm +0.7}_{-1.5}$ & 3.6$\pm$0.4& $12^{\rm +2}_{-2}$ 	& $11 \pm 3$ & $<$0.3 & \dotfill 			& $<$9 		\\
2~~~~JEM-X   & 2005 Mar 25,  22:21:43	& $2.0^{\rm +0.5}_{-0.4}$ & $8^{\rm +5}_{-3}$ 	& 8.7/9 		& $2.8^{\rm +0.6}_{-1.6}$ & $2.6 \pm 0.3$ & $8^{\rm +2}_{-1}$ 	& $9 \pm 2$ & $<$0.3 & 114869 		& $<$11 		 \\
3~~~~JEM-X   & 2005 Apr. 11,  08:53:16	& $1.9^{\rm +0.7}_{-0.5}$ & $12^{\rm +12}_{-12}$ & 13.7/17 	& $4.2^{\rm +1.1}_{-3.4}$ & $4.5 \pm 0.5$ & $8^{\rm +2}_{-1}$ 	& $11 \pm 3$ & $0.7 \pm 0.2$ & 1420269 	& $17 \pm 7 $\\
4~~~~JEM-X*   & 2005 Apr. 17,  06:18:54	& $2.5^{\rm +0.5}_{-0.4}$ & $8^{\rm +3}_{-2}$ 	& 18.4/22 		& $5.5^{\rm +0.7}_{-2.1}$ & $12.6 \pm 1.0$ & $11^{\rm +2}_{-2}$ 	& $23 \pm 3$ & $0.4 \pm 0.2$ & 509114	& $7.7 \pm 4$ 	 \\
5~~~~BAT   & 2007 Jan. 22,  06:12:54 	& $2.4^{\rm +0.8}_{-0.5}$ & $8^{\rm +5}_{-4}$ 	& 5.2/7 & $5.8^{\rm +1.7}_{-2.5}$ & $>$4.7                 & \dotfill 	&$>$8 & \dotfill & \dotfill 	& \dotfill 	 \\
6~~~~XRT   & 2007 Feb. 16,  22:59:28 	& \dotfill			  & \dotfill		 	& \dotfill 		& $2.7^{\rm +0.8}_{-0.8}$ 	  & $3.3 \pm 0.6$  & $13^{\rm +6}_{-5}$         & $12 \pm 6$ & $0.8 \pm 0.1$ & 	2220459& $29 \pm 12$ 	 \\
7~~~~JEM-X   & 2007 Mar 02,  08:42:34 	& $1.6^{\rm +0.3}_{-0.3}$ & $15^{\rm +8}_{-5}$ 	& 9.1/13 		& $3.3^{\rm +0.4}_{-1.5}$ & $5.3 \pm 0.5$ & $16^{\rm +2}_{-3}$ 	& $16 \pm 3$ & $0.7 \pm 0.2$ & 1158185 	& $20 \pm 6$ 	 \\
8~~~~JEM-X   & 2007 Mar 03,  15:51:05 	& $1.9^{\rm +0.3}_{-0.3}$ & $11^{\rm +4}_{-3}$ 	& 11.6/12 		& $3.5^{\rm +0.5}_{-1.2}$ & $3.9 \pm 0.4$ & $11^{\rm +1}_{-2}$     & $11 \pm 2$ & $1.0 \pm 0.2$ & 112057 	& $29 \pm 7$ 	 \\
9~~~~JEM-X   & 2007 Mar. 06,  22:35:16 	& $1.6^{\rm +0.4}_{-0.3}$ & $16^{\rm +13}_{-7}$ & 9.1/11& $3.6^{\rm +0.6}_{-2.3}$ & $4.3 \pm 0.5$ & $10^{\rm +3}_{-2}$ 	& 12$\pm$2 & 1.3$\pm$0.2 & 283423 	& $36 \pm 8$\\ 
10~~JEM-X   & 2007 Mar. 09,  17:28:56 	& $2.8^{\rm +3.1}_{-1.0}$ & $4^{\rm +6}_{-4}$ 	& 5.9/9	& $2.8^{\rm +1.2}_{-2.5}$ & $2.5 \pm 0.5$ & $12^{\rm +4}_{-2}$ 	& 9$\pm$4 & 1.2$\pm$0.2 & 240790 	& $43 \pm 20$\\
11~~JEM-X   & 2007 Mar. 15,  16:01:05	& $1.7^{\rm +0.5}_{-0.4}$ & $14^{\rm +12}_{-14}$ & 8.1/10 & $3.1^{\rm +0.8}_{-2.3}$ & 2.5$\pm$0.4 & $11^{\rm +2}_{-2}$ 	& $8 \pm 3$ & $1.8 \pm 0.2$ & 513094 	& $58 \pm 16$ \\
12~~JEM-X   & 2007 Mar 16,  14:09:14	& $2.2^{\rm +1.0}_{-0.6}$ & $7^{\rm +6}_{-7}$ 	& 5.3/8 		& $2.2^{\rm +0.6}_{-1.9}$ & 2.0$\pm$0.3 & $12^{\rm +4}_{-3}$ 	& $9 \pm 3$ & $1.4 \pm 0.2$ & 79685 		& $65 \pm 20$ 	 \\
13~~JEM-X   & 2007 Mar 19,  01:15:03	& $1.7^{\rm +0.3}_{-0.3}$ & $15^{\rm +8}_{-5}$ 	& 3.6/13 		& $3.9^{\rm +0.7}_{-2.5}$ & 3.6$\pm$0.4 & $10^{\rm +3}_{-3}$ 	& $11 \pm 2$ & $1.4 \pm 0.2$ & 212715 	& $35 \pm 8$ 	 \\
14~~XMM  & 2007 Mar 31,  01:15:15	& $1.9^{\rm +0.6}_{-0.4}$ & $7^{\rm +3}_{-2}$ 	& 8.5/9 		& $1.1^{\rm +0.2}_{-0.6}$ & 2.5$\pm$0.3 & $19^{\rm +2}_{-2}$ 	& $21 \pm 5$ & $0.6 \pm 0.1$ & 1036812 	& $54 \pm 17$ 	 \\
15~~XMM  & 2007 Apr 02,  02:39:03		& $2.2^{\rm +0.4}_{-0.3}$ & $6^{\rm +2}_{-2}$ 	& 25.5/21 		& $1.3^{\rm +0.2}_{-0.3}$ & $3.6 \pm 0.4$ & $21^{\rm +2}_{-2}$ 	& $28 \pm 5$ & $0.7 \pm 0.1$ & 177828 	& $54 \pm 10$ \\
\noalign{\smallskip}
\hline
\end{tabular}}
\medskip
$^a$  Number of the burst, and instrument that detected it. *~designates the burst that was also detected by ISGRI;  $^b$~blackbody temperature at the peak of the burst, assuming $N_{\rm H}=12 \times 10^{22}$~cm$^{-2}$; $^c$~Blackbody radius at the peak assuming a distance of 7~kpc to the source; $^d$~{unabsorbed bolometric flux (0.1--100~keV) at the peak in units of $10^{-8}$ \ergperseccm.} $^e$  {Fluence of the burst in units of $10^{-7}$ \ergpercm}; $^f$~{e-folding decay time fitted on the light curve;} $^g$~{e-folding decay time calculated with $\tau_{\rm calc}\equiv f_{\rm b}/F_{\rm peak}$}; $^h$~{unabsorbed bolometric persistent flux (0.1--100~keV) prior to the burst in units of $10^{-9}$ \ergperseccm}; $^i$~{time ellapsed since last detected burst.} $^j$  {Ratio of persistent flux to burst flux: $\gamma \equiv F_{\rm pers}/F_{\rm peak}$.}
\end{table}