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Table 2.
Parameters for the fit to the γ-ray light curve of the 2015 flaring episode.
| Nexp | Ai (×106) | tri [days] | tdi [days] | tci [year] | χ2/d.o.f. | ξ |
|---|---|---|---|---|---|---|
| 3 | 0.9 (0.2) | 58 (12) | 18.2 (7.7) | 2015.605 (0.022) | 5.1 | 0.5 |
| 0.7 (0.1) | 49 (35) | 86 (48) | 2015.941 (0.122) | −0.3 | ||
| 0.15 (0.07) | 3.2 (6.4) | 490 (340) | 2016.332 (0.018) | −1.0 |
Notes. The resulting reduced χ2-statistic for the fit is shown, and also the computed symmetry factor ξi for each subflare. The result can be seen in Fig. 7.
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