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Table 1

Observation IDs and light curve properties of all 15 type I X-ray bursts.

Burst No. NICER Burst onset Peak rate(c) Dip duration(d) Dip count(e)
# (Obs Id) (MJD) (104 C S−1) (s) (%)
1 1050300108 57 994.37393 2.15 0.6 ± 0.1 47.5 ± 0.1
2 1050300108 57 994.46448 1.56
3 1050300109 57 995.22557 2.28 0.7 ± 0.1 31.3 ± 0.1
4 1050300109 57 995.34162 2.08 0.7 ± 0.1 41.4 ± 0.1
5 1050300109 57 995.60600 1.89 1.0 ± 0.1 61.1 ± 0.1
6 2050300104 58 641.29573 2.52 1.9 ± 0.1 8.4 ± 0.1
7 2050300108 58 646.84015 1.96 2.0 ± 0.1 −0.9 ± 0.1
8 2050300110 58 648.32669 2.25 2.7 ± 0.1 −1.0 ± 0.1
9 2050300115(a) 58 655.09203 2.59 1.7 ± 0.1 15.5 ± 0.1
10 2050300119(b) 58 660.31327 2.60 1.7 ± 0.1 8.3 ± 0.1
11 2050300119 58 660.77147 2.58 1.5 ± 0.1 17.7 ± 0.1
12 2050300120(a) 58 661.78614 2.22 1.0 ± 0.1 27.5 ± 0.1
13 2050300122(a) 58 663.98438 2.57 1.1 ± 0.1 20.4 ± 0.1
14 2050300124 58 665.59405 2.54 1.6 ± 0.1 13.4 ± 0.1
15 4680010101 59 336.61230 2.57 1.7 ± 0.1 13.6 ± 0.1

Notes. Bursts #1 and #1-5 are studied in Keek et al. (2018) and Strohmayer et al. (2019), respectively. (a)The X-ray bursts in the UFA event file. (b)The tail of burst #10 was truncated due to a data gap. (c)The peak rates with persistent emission subtracted are measured from the 0.1 s light curves in the energy range of 0.5–10 keV. (d)The dip duration of the 0.1 s light curves in the energy range of 3–10 keV. (e)The ratio of minimum count rate during the dip to peak count rate in 3–10 keV.

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