Table 2.
Results of the continuum modelling for all bursts with the fa model in XSPEC.
# | ObsID | Date | Γ | Norm | kTBB | Radius | LX | C-STAT |
---|---|---|---|---|---|---|---|---|
1 | 1050300108 | 2017-08-29T08:53:16.07 | ![]() |
![]() |
![]() |
![]() |
6.3 ± 0.3 | 389.7 (2.6) |
2 | 1050300108 | 2017-08-29T11:03:40.41 | ![]() |
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![]() |
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7.6 ± 0.4 | 342.6 (0.3) |
3 | 1050300109 | 2017-08-30T05:19:44.92 | ![]() |
![]() |
![]() |
![]() |
5.7 ± 0.2 | 333.8 (0.6) |
4 | 1050300109 | 2017-08-30T08:06:51.31 | ![]() |
![]() |
![]() |
![]() |
6.7 ± 0.3 | 403.4 (3.1) |
5 | 1050300109 | 2017-08-30T14:27:36.30 | ![]() |
![]() |
![]() |
![]() |
6.3 ± 0.4 | 353.9 (1.1) |
6 | 2050300104 | 2019-06-07T06:56:50.46 | ![]() |
![]() |
![]() |
![]() |
4.3 ± 0.1 | 398.1 (5.3) |
7 | 2050300108 | 2019-06-12T20:00:34.79 | ![]() |
![]() |
![]() |
![]() |
3.3 ± 0.1 | 351.5 (4.8) |
8 | 2050300110 | 2019-06-14T07:41:08.28 | ![]() |
![]() |
![]() |
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2.8 ± 0.1 | 290.5 (5.9) |
9 | 2050300119 | 2019-06-26T07:21:30.42 | ![]() |
![]() |
![]() |
![]() |
4.1 ± 0.1 | 390.1 (6.7) |
10 | 2050300119 | 2019-06-26T18:21:25.29 | ![]() |
![]() |
![]() |
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5.0 ± 0.1 | 372.4 (2.9) |
11 | 2050300124 | 2019-07-01T14:05:57.58 | ![]() |
![]() |
![]() |
![]() |
4.7 ± 0.1 | 398.5 (4.3) |
12 | 4680010101 | 2021-05-02T14:35:35.51 | ![]() |
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4.5 ± 0.1 | 407.9 (5.8) |
Notes. The best-fit spectral parameters of the burst peak emission for the fa model that also accounts for the underlying persistent emission. The labels are the same as in Table 1. The bolometric luminosity is computed between 0.2 and 20 keV, assuming a distance of 8 kpc and expressed in units of 1038 erg s−1. The radius parameter is expressed in units of 102 km. The errors on the best-fit parameters are given at the 90% confidence levels.
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