\begin{table}%t1 \caption {\label{t1}The 18 type-I X-ray bursts' rise time, decay time, the temperature of BB, and the radius, bolometric flux, fluency, characteristic time scale~$\tau$, and bolometric flux of the persistent flux.} %\centerline {\begin{tabular}{cccccccccccccccccc} \hline \hline \noalign{\smallskip} No& OBSID & Time & Intensity &$t_{r}$ &$t_{d}$ &$T_{\rm bb}$ &$R_{\rm bb}$ &$F_{\rm pk}$ &$E_{\rm b}$ &$\tau$ &$F_{\rm per}$\\ & & (MJD) &(cts~s$^{-1}$) &(s) &(s) &(keV) &(km) &($10^{-8}$) &($10^{-7}$) & (s)&($10^{-9}$)\\ \hline \noalign{\smallskip} 1& 91050-02-01-00 &53514.297601 &4055&4&12.7&$2.46^{\rm +0.11}_{-0.11}$ &$7.7^{\rm +0.7}_{-0.6}$ &6.0 &12 &20.0 &3.30\\[0.5mm]%\hline 2 &91050-02-05-00 &53521.108180 &1896 &6&13.9&$2.25^{\rm +0.15}_{-0.14}$ &$6.0^{\rm +0.8}_{-0.7}$&2.56 &5.36&20.9 &2.57\\[0.5mm]%\hline 3 &93442-01-03-01 &54624.293851 & 2498&6&21.7&$2.33^{\rm +0.14}_{-0.13}$ &$6.6^{\rm +0.8}_{-0.7}$&3.61 &10 &27.3&7.42\\[0.5mm]%\hline 4 &93442-01-03-05 &54628.026895 &3443 &6&15.1&$2.76^{\rm +0.17}_{-0.16}$ &$5.7^{\rm +0.6}_{-0.5}$&5.01 &10.64& 27.7&8.00\\[0.5mm]%\hline 5 &93442-01-03-06 &54629.213273 &2562 &5&21.5&$2.54^{\rm +0.17}_{-0.16}$ &$5.7^{\rm +0.8}_{-0.6}$&3.74 &9.12&21.2 &8.02\\[0.5mm]%\hline 6 &93442-01-04-00 &54630.523574 &3378 &5&15.6&$2.79^{\rm +0.17}_{-0.16}$ &$5.5^{\rm +0.7}_{-0.6}$&5.15 &10.72& 20.8 &8.85\\[0.5mm]%\hline 7& 93442-01-04-01 &54632.008828 &2473 &6&20.6&$2.35^{\rm +0.16}_{-0.15}$ &$6.4^{\rm +1.0}_{-0.7}$&3.54 &9.12 &25.8 &9.25\\[0.5mm]%\hline 8 & 93442-01-04-04&54634.909141 &2457 &7&21.4&$2.53^{\rm +0.20}_{-0.18}$ &$5.6^{\rm +0.9}_{-0.7}$&3.51 &9.12&26.0 &9.21\\[0.5mm]%\hline 9\tablefootmark{*}& 93442-01-08-06&54664.351270 & 5789 &2&6.7 &$2.32^{\rm +0.10}_{-0.09}$&$10.1^{\rm +0.8}_{-0.7}$&8.23 &7.36 & 8.9 &5.42\\[0.5mm]%\hline 10&93442-01-08-06& 54664.486930 & 3563 &6&5.6 &$2.41^{\rm +0.13}_{-0.12}$&$7.3^{\rm +0.8}_{-0.7}$&4.99 &4.08 & 8.18 &5.15\\[0.5mm]%\hline 11\tablefootmark{*}& 93442-01-09-00& 54666.359905 & 5058 &2&7.8&$2.35^{\rm +0.09}_{-0.09}$ &$9.8^{\rm +0.8}_{-0.7}$&8.18 &6.72 & 8.21&5.86\\[0.5mm]%\hline 12& 93442-01-10-05& 54676.784407&2989&4&12.2&$2.36^{\rm +0.12}_{-0.11}$ &$7.0^{\rm +0.7}_{-0.6}$&4.16 &7.2 &17.3&2.61\\[0.5mm]%\hline 13& 93442-01-12-05& 54692.425935 &2898 &4&12.0&$2.41^{\rm +0.14}_{-0.13}$ &$6.6^{\rm +0.8}_{-0.6}$&4.11 &6.8 &16.5&2.50\\[0.5mm]%\hline 14& 93442-01-15-04& 54712.285321 &3792 &3&10.6&$2.76^{\rm +0.16}_{-0.15}$ &$6.0^{\rm +0.6}_{-0.5}$&5.85 &6.08 &14.4&1.79\\[0.5mm]%\hline 15 &93442-01-15-05& 54713.359592 &3681 &3&10.9&$2.62^{\rm +0.13}_{-0.13}$ &$6.6^{\rm +0.6}_{-0.5}$&5.67 &7.92 &14.0&2.00\\[0.5mm]%\hline 16 &93442-01-16-06 &54717.394303 &4072 &3&9.5 &$3.25^{\rm +0.19}_{-0.17}$ &$4.8^{\rm +0.4}_{-0.4}$&7.01 &7.92 &11.3&1.70\\[0.5mm]%\hline 17 &93442-01-17-01& 54723.019835 &3875 &3&8.5 &$2.98^{\rm +0.18}_{-0.16}$ &$5.4^{\rm +0.5}_{-0.5}$&6.29 &6.56 &10.4&1.44\\[0.5mm]%\hline 18\tablefootmark{*} &93442-01-17-05 &54726.704638 & 4430&3&8.0 &$2.41^{\rm +0.10}_{-0.10}$&$8.6^{+0.9}_{-0.8}$&6.92 &8.16 & 11.8 &1.36\\ \hline \end{tabular}} \tablefoot{1 crab is roughly 2500~counts/PCU/s in the 2--60~keV band. The bolometric flux and fluence are presented in the energy band 1.5--30~keV, and in unit of $\rm erg~cm^{2}~s^{-1}$.} \tablefoottext{*}{Burst shows photosphere radius expansion.} \end{table}