Table 10
Output from the individual MCMC analyses of the light curves with the 5 highest energy flares.
| Flare # | Timing ± 1-σ | Amplitude ± 1-σ | Duration ± 1-σ | Flare energy ± error (erg) | ||||
|---|---|---|---|---|---|---|---|---|
| [JD – 2 450 000] | [%] | (days) | (erg) | |||||
| 1 | 7655.97363 | 0.0038 | 0.635 | 0.39 | 0.00759 | 0.0045 | 8.41 E+31 | 5.08e+31 |
| 2 | 7659.38103 | 0.00051 | 0.846 | 0.065 | 0.04508 | 0.0072 | 6.64 E+32 | 4.02e+32 |
| 3 | 7667.12545 | 0.00052 | 1.276 | 0.092 | 0.0264 | 0.0034 | 5.79 E+32 | 3.50e+32 |
| 4 | 8021.16339 | 0.00052 | 0.148 | 0.093 | 0.0248 | 0.0029 | 6.41 E+31 | 3.87e+31 |
| 5 | 8046.8164 | 0.0011 | 0.346 | 0.048 | 0.030 | 0.016 | 1.81 E+32 | 1.09e+32 |
Notes. Timing, amplitude, and duration are measured through a MCMC analysis of the corresponding light curves, while the flare energy is computed by applying Eq. (20) and its error is estimated to be ± 60% of the flare energy following the recommendations of Shibayama et al. (2013).
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