Table 1.
Input model parameters for the EC models of PKS 1510–089 emission for the low state in close and far scenarios.
| γmin | γb | γmax | n1 | n2 | B | K | δ | Γ | r | R | |
|---|---|---|---|---|---|---|---|---|---|---|---|
| Low state (close) | 2.5 | 130 | 3 × 105 | 1.9 | 3.5 | 0.35 | 3 × 104 | 25 | 20 | 7.0 × 1017 | 2.0 × 1016 |
| Low state (far) | 2 | 300 | 3 × 105 | 1.9 | 3.7 | 0.05 | 80 | 25 | 20 | 3.0 × 1018 | 3.0 × 1017 |
| 2012 | 3 | 900 | 6.5 × 104 | 1.9 | 3.85 | 0.12 | 20 | 20 | 20 | 3.1 × 1018 | 3.0 × 1017 |
| 2015, Period A | 1 | 150 & 800 | 4 × 104 | 1 & 2 | 3.7 | 0.23 | 3.0 × 104 | 25 | 20 | 6.0 × 1017 | 2.8 × 1016 |
| 2015, Period B | 1 | 150 & 500 | 3 × 104 | 1 & 2 | 3.7 | 0.34 | 2.6 × 104 | 25 | 20 | 6.0 × 1017 | 2.8 × 1016 |
Notes. For comparison, model parameters obtained from the 2012 high state (Aleksić et al. 2014) and 2015 flare (Ahnen et al. 2017a) are also quoted. The individual columns are minimum, break, and maximum electron Lorentz factor (γmin, γb, γmax, respectively); slope of the electron energy distribution below and above γb (n1 and n2, respectively); magnetic field in G (B); normalization of the electron distribution in units of cm−3 (K); Doppler, Lorentz factor, distance, and radius of the emission region (δ, Γ, r (in cm), R (in cm), respectively).
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