Table 8.
Fraction of emission at optical (R-band) which originated from the core emission.
| (1) | (2) | (3) | (4) | (5) |
|---|---|---|---|---|
| Source name | Campaign/state | Radio – optical long-term | Polarisation | SED Modelling |
| VER J0521+211 | 2013 | > 0.36 | [0.05–0.22] | 0.87 |
| PKS 1424+240 { | 2014 | > 0.0 | [0.31–0.72] | 0.94 |
| 2015 | > 0.0 | [0.28–0.67] | 0.96 | |
| 1ES 1727+502 | 2015 | > 0.26 | [0.18–0.70] | 0.63 |
| 1ES 1959+650 { | 2016/low | > 0.52 | [0.14–0.56] | 0.44 |
| 2016/intermediate | > 0.52 | [0.21–0.87] | 0.49 | |
| 2016/high | > 0.52 | [0.21–0.89] | 0.41 | |
| 1ES 2344+514 | 2016 | > 0.06 | [0.08–0.35] | 0.63 |
Notes. Columns: (1) Source name. (2) Observation campaign/state. (3), (4) and (5) Ratio between core flux and total flux obtained from radio-optical long-term light curve, polarisation analysis, and two-component SED modelling. The fractions are calculated using the methods described in Sects. 3.2.1 and 3.3. The results from the SED modelling are also presented for comparison.
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