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Table 2.
Broken power-law model parameters.
| Epoch 1 | Epoch 2 | Epoch 3 | Epoch 4 | Epoch 5 | |
|---|---|---|---|---|---|
| 2017 | 2017 | 2017 | 2018 | 2021 | |
| Sep 21–23 | Dec 9–10 | Dec 21–22 | Jan 8–9 | Aug 8–12 | |
| R [cm] | 1017 | ||||
| δ | 40 | ||||
| γmin | 10 | ||||
| γmax | 108 | ||||
| B [mG] | 1.67 | 3.12 | 2.58 | 3.40 | 1.97 |
| p1 | 2.25 | 2.46 | 2.40 | 2.55 | 2.32 |
| p2 | 4 | ||||
Notes. Parameters set for the modelling of the blazar SEDs assuming an electron distribution following the broken power-law model: these are assumed to be equal for each source we analysed. The different epochs are those of Hota et al. (2024), as discussed in the text.
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