Table 1.
Parameters for the fit to the γ-ray light curve of the 2008 flaring episode to functions of shape given by Eq. (1).
| Nexp | Ai (×106) | tri [days] | tdi [days] | tci [year] | χ2/d.o.f. | ξ |
|---|---|---|---|---|---|---|
| 4 | 2.0 (0.1) | 17.8 (4.3) | 36.4 (3.2) | 2008.698 (0.014) | 2.8 | −0.3 |
| 0.4 (0.1) | < 2.6 | 37.8 (20) | 2008.968 (0.006) | −0.9 | ||
| 0.2 (…) | < 26 | … | 2009.085 (…) | −1.0 | ||
| 0.09 (…) | < 200 | … | 2009.430 (…) | −1.0 | ||
| 5 | 1.7 (0.4) | 25.7 (2.1) | < 4.4 | 2008.728 (0.008) | 2.3 | 0.7 |
| 1.5 (0.4) | 5.3 (5.0) | 27.9 (4.7) | 2008.758 (0.007) | −0.7 | ||
| 0.5 (0.1) | 4.6 (2.9) | 37.7 (21) | 2008.965 (0.012) | −0.8 | ||
| 0.2 (4 × 103) | < 17.2 | … | 2009.086 (…) | −1.0 | ||
| 0.09 (4 × 101) | < 290 | … | 2009.432 (44) | −1.0 | ||
Notes. The resulting reduced χ2-statistic for the fit is shown, and also the computed symmetry factor ξi for each subflare. Some values could not be computed. Upper limits are indicated with ‘< ’. The result can be seen in Fig. 7.
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