Table 5
Model parameters.
| Reference | This campaign | Albert et al. (2007b) | Tavecchio et al. (2010) | Acciari et al. (2011b) | |||||
| Model reference | (1) | (2) | (3) | (1) | (3) | ||||
| Flux level | low | high | low | high | low | highb | ... | low | high |
|
|
|||||||||
| B [G] | 0.07 | 0.05 | 0.09 | 0.10 | 0.08 | 0.1 | 0.09 | 0.03 | |
| δ | 20 | 26 | 29 | 8 | 15 | 25 | 13 | 20 | |
| Rem [1015 cm] | 3 | 4 | 9 | 5 | 10 | 4 | 10 | ||
| Racc [1013 cm] | ... | ... | 8 | 13 | ... | ... | ... | ... | ... |
|
|
|||||||||
| Ka [105 cm-3] | 4.5 | 1.9 | 0.2 | 0.1 | ~0.5 | ~0.4 | 0.3 | ~0.4 | |
| e 1 | 2.3 | 2.5 | 2.3 | 2.2 | 2 | 2.5 | 2.3 | ||
| e 2 | 3.4 | 3.2 | 3.5 | 3.3 | 3.2 | 3.2 | 3.2 | ||
| γ min | 1 or 4000 | 1800 | 550 | ~2500 | ~1500 | 1 (8000)c | ~200 | ||
| γbreak [104] | 5 | 8 | 10 | 3 | ~15 | 1 | ~40 | ~50 | |
| γmax [106] | 0.7 | 1.5 | 6.3 | 1.5 | ~0.8 | ~1.6 | 0.7 | ~2.0 | |
Notes.See text or reference for an explanation of the models. The used data sets and their simultaneity are discussed in the text.
Note that K is given for the acceleration region at γmin in Weidinger & Spanier (2010), whereas the value is defined for the emission region at γmin = 1 for the other two models.
See footnote 15.
Fit has been performed on optical data not corrected for the host galaxy. See also footnote 16.
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