Table 1.
Characteristics of EVPA rotations of the selected blazars.
| 1 | 2 | 3 | 4 | 5 | 6 |
|---|---|---|---|---|---|
| B1950 | Common | AGN | SED peak | z | δvar |
| name | name | type | classification | ||
| 0716+714 | S5 0716+71 | BL Lac | ISP | 0.310 | 23.3 ± 3.6 |
| 0851+202 | OJ 287 | BL Lac | LSP | 0.306 | 6.4 ± 1.9 |
| 1553+113 | PG 1553+113 | BL Lac | HSP | 0.360 | ∼1.4 |
| 2230+114 | CTA 102 | FSRQ, HPQ | LSP | 1.032 | 37.5 ± 6.7 |
| 2251+158 | 3C 454.3 | FSRQ, HPQ | LSP | 0.859 | 28.8 ± 2.2 |
Notes. Column 1 – B1950 name of the source, Col. 2 – common name of the source, Col. 3 – AGN type of the source, Col. 4 — SED peak classification, Col. 5 – redshift, z, according to the NASA Extragalactic Database2, Col. 6 – estimate of the Doppler factor, δvar, from Weaver et al. (2022) except PG 1553+113 (Lico et al. 2020).
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