Table 3.
Accretion state and radio to millimetre spectral indices.
| Obs. | State | Slope 1 | Slope 2 | Jet break |
|---|---|---|---|---|
| 1 | Hard/Intermediate | 0.11 ± 0.06 | –0.15 ± 0.06 | ~100 GHz |
| 1 | Hard/Intermediate | 0.11 ± 0.06 | –1.4 ± 0.7 | ~250 GHz |
| 2a | Soft | –1.76 ± 0.25 | ≲5 GHz | |
| 2b | Soft | –0.19 ± 0.09 | ≲5 GHz | |
| 3 | Hard/Intermediate | 0.70 ± 0.17 | –0.21 ± 0.01 | ~30 GHz |
| 3 | Hard/Intermediate | 0.34 ± 0.05 | –0.21 ± 0.01 | ~100 GHz |
Notes. For obs 1 and 3, we obtained two jet spectral breaks per observation by taking into account different scenarios (see text). The two values are considered as lower and upper limits of the break for each observation. The true value very likely lies between these two extremes.
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