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Table 1:

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.

No
OBSID Time Intensity tr td $T_{\rm bb}$ $R_{\rm bb}$ $F_{\rm pk}$ $E_{\rm b}$ $\tau $ $F_{\rm per}$
    (MJD) (cts s-1) (s) (s) (keV) (km) (10-8) (10-7) (s) (10-9)
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
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
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
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
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
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
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
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
9* 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
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
11* 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
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
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
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
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
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
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
18* 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

Notes. 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 $\rm erg~cm^{2}~s^{-1}$.

(*) Burst shows photosphere radius expansion.


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