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Table 4.
Modeled parameters of γ-ray SEDs for all the segments identified in Fig. 1.
| Various | F0.1−300 GeV | Luminosity | PowerLaw | TS | TScurve | ||
|---|---|---|---|---|---|---|---|
| states | (10−8 ph cm−2 s−1) | (1048 erg s−1) | ΓPL | ||||
| A | 4.10 ± 0.50 | 0.25 | −1.90 ± 0.06 | – | – | 570.20 | – |
| B | 4.90 ± 0.60 | 0.80 | −2.27 ± 0.08 | – | – | 313.00 | – |
| C | 5.10 ± 0.81 | 0.93 | −2.24 ± 0.10 | – | – | 173.22 | – |
| D | 5.40 ± 0.81 | 1.04 | −2.35 ± 0.10 | – | – | 178.32 | – |
| E | 5.20 ± 0.55 | 2.92 | −2.21 ± 0.06 | – | – | 551.28 | – |
| LogParabola | |||||||
| α | β | ||||||
| A | 3.60 ± 0.70 | 0.22 | 1.81 ± 0.12 | 0.03 ± 0.03 | – | 569.48 | −0.72 |
| B | 4.90 ± 0.60 | 0.81 | 2.27 ± 0.08 | 0.00 ± 0.00 | – | 313.01 | 0.01 |
| C | 4.70 ± 0.96 | 0.84 | 2.19 ± 0.13 | 0.05 ± 0.07 | – | 173.64 | 0.42 |
| D | 5.40 ± 0.81 | 0.96 | 2.35 ± 0.10 | 0.00 ± 0.00 | – | 178.30 | 0.02 |
| E | 5.20 ± 0.55 | 2.45 | 2.21 ± 0.06 | 0.00 ± 0.00 | – | 551.24 | −0.08 |
| Broken PowerLaw | Ebreak | ||||||
| Γ1 | Γ2 | [GeV] | |||||
| A | 3.70 ± 0.70 | 0.21 | −1.77 ± 0.17 | −1.98 ± 0.11 | 1.43 ± 0.74 | 569.44 | −0.76 |
| B | 5.30 ± 0.30 | 1.03 | −2.44 ± 0.83 | −2.16 ± 0.09 | 0.64 ± 0.25 | 315.26 | 2.26 |
| C | 3.60 ± 1.20 | 1.08 | −1.97 ± 0.24 | −2.64 ± 0.36 | 1.78 ± 0.16 | 144.38 | −28.84 |
| D | 6.20 ± 0.87 | 1.16 | −2.64 ± 0.14 | −1.86 ± 0.16 | 1.41 ± 0.13 | 186.32 | 8.00 |
| E | 5.80 ± 2.00 | 3.02 | −2.40 ± 0.45 | −2.04 ± 0.06 | 1.00 ± 0.32 | 560.03 | 8.75 |
Notes. Column 3 shows the isotropic γ-ray luminosity during the various segments, which is lower than the Eddington luminosity (∼1050 erg s−1) of the source, as discussed in Sect. 3.4.
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