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Home All issues Volume 696 (April 2025) A&A, 696 (2025) A139 Full HTML
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Table A.1.

Burst observations.

Burst No. Obs-ID Date Time MJD Peak Rate a Δtb
# (YYYY-MM-DD) (UT) (TT) (104 c s−1) (s)
1 1050300108 2017-08-29 08:58:27 57994.37393 2.15 0.3-0.8
2 1050300108 2017-08-29 11:08:51 57994.46448 1.56 0.4-1.4
3 1050300109 2017-08-30 05:24:49 57995.22557 2.28 0.4-0.8
4 1050300109 2017-08-30 08:11:55 57995.34162 2.08 0.4-0.8
5 1050300109 2017-08-30 14:32:38 57995.60600 1.89 0.9-1.4
6 2050300104 2019-06-07 07:05:51 58641.29573 2.52 0.5-1.1
7 2050300108 2019-06-12 20:09:49 58646.84015 1.96 0.1-0.8
8 2050300110 2019-06-14 07:50:25 58648.32669 2.25 0.4-1.4
9 2050300115 c 2019-06-21 02:12:31 58655.09203 2.59 0.2-0.7
10 2050300119 2019-06-26 07:31:06 58660.31327 2.60 0.3-1.0
11 2050300119 d 2019-06-26 18:30:54 58660.77147 2.58 0.4-1.1
12 2050300120 c 2019-06-27 18:52:02 58661.78614 2.22 0.8-1.4
13 2050300122 c 2019-06-29 23:37:30 58663.98438 2.57 0.4-1.0
14 2050300124 2019-07-01 14:15:25 58665.59405 2.54 0.4-1.1
15 4680010101 2021-05-02 14:41:42 59336.61230 2.57 0.6-1.2

Notes.

(a)

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.

(b)

The start/end times (relative to burst onset) used to extract PRE phase spectra.

(c)

The X-ray bursts in the ufa event file.

(d)

The tail of burst #10 was truncated due to data gap.

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