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Table 1.
Parameters used for the modelling of the extreme blazar datasets in scenarios I, II, and III.
| 1ES 0229+200 | 1ES 0347−121 | RGB J0710+591 | 1ES 1101−232 | 1ES 1218+304 | |
|---|---|---|---|---|---|
| Scenario I | |||||
| δ | 50 | 30 | 40 | 50 | 60 |
| Rsrc [1016cm] | 1.8 | 4.7 | 2.0 | 3.0 | 1.1 |
| B [mG] | 4.4 | 3.7 | 7.9 | 8.9 | 8.4 |
| σrad ( ≡ σ ) | 1.0 × 10−4 | 1.4 × 10−4 | 5.0 × 10−4 | 1.6 × 10−3 | 9.8 × 10−5 |
| γe, min | 3.0 × 104 | 1.8 × 104 | 2.4 × 104 | 3.0 × 104 | 5.0 × 103 |
| γe, max | 2.9 × 106 | 1.5 × 106 | 1.1 × 106 | 7.6 × 105 | 5.0 × 105 |
| ne [cm−3] | 2.9 × 10−2 | 2.7 × 10−2 | 2.8 × 10−2 | 1.0 × 10−2 | 0.69 |
| Scenario II | |||||
| δ | 50 | 50 | 50 | 50 | 60 |
| Rsrc [1016cm] | 2.3 | 1.6 | 1.9 | 4.5 | 1.4 |
| B [mG] | 4.4 | 6.2 | 9.8 | 8.9 | 8.4 |
| σrad | 1.9 × 10−4 | 1.1 × 10−4 | 1.2 × 10−3 | 4.0 × 10−3 | 1.4 × 10−4 |
| σrad/σ | 11 | 29 | 270 | 64 | 11 |
| γe, min | 1.2 × 104 | 1.8 × 103 | 1.8 × 103 | 6.0 × 103 | 1.8 × 103 |
| γe, max | 2.9 × 106 | 9.1 × 105 | 8.6 × 105 | 7.6 × 105 | 5.0 × 105 |
| ne [cm−3] | 4.2 × 10−2 | 0.83 | 0.24 | 2.1 × 10−2 | 1.3 |
| Scenario III | |||||
| δ | 50 | 50 | – | 50 | – |
| Rsrc [1016cm] | 1.3 | 0.9 | – | 7.0 | – |
| B [mG] | 4.4 | 6.2 | – | 4.5 | – |
| σrad | 1.0 × 10−4 | 9.0 × 10−5 | – | 4.0 × 10−3 | – |
| σrad/σ | 270 | 23 | – | 720 | – |
| γe, min | 1.8 × 103 | 1.8 × 103 | – | 1.8 × 103 | – |
| γe, max | 2.9 × 106 | 9.1 × 105 | – | 7.6 × 105 | – |
| ne [cm−3] | 0.13 | 0.29 | – | 8.2 × 10−3 | |
Notes. The observables used as input for the modelling and parameters of the proton population can be found in Table D.1.
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