Table 7.
Results obtained from the one-zone SSC and two-component SED modelling.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|---|---|---|---|---|---|---|---|---|---|
| Source name | Campaign/ | Model | LB | Le | Lp |
 |
CD | log νsync | log νIC |
| state | (×1043 erg s−1) | (Hz) | |||||||
| One-zone | 0.19 | 129 | 13.6 | 0.001 | 2.05 | 15.12 | 24.17 | ||
| VER J0521+211 | 2013 | ||||||||
| 2-comp | 82.8 | 40.9 | 46.8 | 0.9 | 1.71 | 14.38 | 24.56 | ||
| One-zone | 2.79 | 624 | 68.1 | 0.004 | 0.41 | 15.23 | 24.02 | ||
| 2014 | |||||||||
| 2-comp | 520 | 198 | 176 | 2.4 | 0.55 | 14.70 | 24.82 | ||
| PKS 1424+240 | |||||||||
| One-zone | 1.98 | 697 | 52.3 | 0.003 | 0.58 | 15.08 | 24.02 | ||
| 2015 | |||||||||
| 2-comp | 520 | 219 | 199 | 1.1 | 0.43 | 14.67 | 24.63 | ||
| One-zone | 0.02 | 5.5 | 1.0 | 0.003 | 0.33 | 18.41 | 25.70 | ||
| 1ES 1727+502 | 2015 | ||||||||
| 2-comp | 1.9 | 2.1 | 3.8 | 4.5 | 0.33 | 18.28 | 25.87 | ||
| One-zone | 0.16 | 12.8 | 12.4 | 0.01 | 0.21 | 17.59 | 25.36 | ||
| 2016/low | |||||||||
| 2-comp | 5.1 | 5.1 | 4.6 | 25.6 | 0.24 | 17.60 | 25.93 | ||
| One-zone | 0.05 | 17.4 | 9.8 | 0.003 | 0.68 | 17.92 | 25.59 | ||
| 1ES 1959+650 | 2016/intermediate | ||||||||
| 2-comp | 1.3 | 9.8 | 7.5 | 16.7 | 0.59 | 18.04 | 25.71 | ||
| One-zone | 0.04 | 1.4 | 4.2 | 0.003 | 0.65 | 18.62 | 25.82 | ||
| 2016/high | |||||||||
| 2-comp | 1.3 | 10.9 | 2.3 | 3.1 | 0.64 | 18.55 | 25.86 | ||
| One-zone | 0.01 | 11.7 | 3.6 | 0.001 | 0.72 | 18.22 | 25.40 | ||
| 1ES 2344+514 | 2016 | ||||||||
| 2-comp | 2.1 | 2.5 | 2.8 | 3.4 | 0.65 | 18.66 | 25.48 | ||
Notes. Columns: (1) Source name. (2) Observation campaign/state. (3) Model. (4), (5) and (6) Kinetic energy of the magnetic field, electrons, and cold protons of the emission region (core in the case of two-component model), respectively. (7) Ratio between the magnetic field and relativistic electron energy densities. (8) The luminosity ratio between the IC and Synchrotron peak (Compton Dominance parameter). (9) and (10) Observed synchrotron and IC peak frequencies.
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