Table 4
Input model parameters assumed for the SSC model (Maraschi & Tavecchio 2003) shown in Fig. 7.
| Year | γmin | γb | γ max | n 1 | n 2 | B | K | R | δ | |
| [103] | [104] | [105] | [G] | [103 cm-3] | [1016 cm] | |||||
|
|
||||||||||
| 2007a | 3.0 | 5.0 | 200 | 2.0 | 5.0 | 0.15 | 20 | 1.0 | 20 | |
| 2008b | 7.0 | 3.4 | 8.0 | 1.9 | 3.3 (3.5) | 0.048 | 0.7 (0.8) | 3.25 | 26 | |
| 2011/2012I | 10.0 | 4.0 | 7.0 | 2.0 | 3.7 | 0.19 | 10.0 | 1.0 | 20 | |
| 2011/2012II | 10.0 | 3.3 | 4.0 | 2.0 | 3.8 | 0.19 | 13.4 | 0.9 | 20 | |
Notes. The parameters for the SED modeling of previous observations are shown for comparison. The parameters reported for the modeling of the 2008 data consider the high (low) state observed in X-rays, while those listed for the modeling of the 2007 data are based on the MAGIC spectrum that has been corrected for EBL absorption using the model by Kneiske et al. (2002) current at that time.
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