Table 7.
Polarisation parameters for the 19 pulsars in our sample.
| Pulsar | RM | RM Reference | Ip/I | ⟨L⟩/I | ⟨V⟩/I | ⟨∥V∥⟩/I |
|---|---|---|---|---|---|---|
| (rad m−2) | (%) | (%) | (%) | (%) | ||
| J0023+0923 | −6 | Wang et al. (2023a) | 30 | 29 | 3 | 4 |
| J0610−2100 | 33.7 | Spiewak et al. (2022) | 66 | 65 | −6 | 5 |
| J0636+5128 | −7.0 | Wahl et al. (2022) | 35 | 33 | −5 | 6 |
| J1124−3653 | / | / | / | / | 3 | 8 |
| J1513−2550 | / | / | / | / | −8 | 2 |
| J1544+4937 | 10.3 | Wang et al. (2023a) | 15 | 12 | 1 | 2 |
| J1555−2908 | / | / | / | / | 5 | 4 |
| J1628−3205 | / | / | / | / | −2 | 3 |
| J1705−1903 | −5.6 | Spiewak et al. (2022) | 19 | 18 | 1 | 1 |
| J1719−1438 | 17.3 | Spiewak et al. (2022) | 38 | 24 | −27 | 12 |
| J1731−1847 | 21.5 | Spiewak et al. (2022) | 51 | 47 | −20 | 17 |
| J1745+1017 | 24.2 | Wang et al. (2023a) | 48 | 40 | −23 | 17 |
| J1959+2048 | −70.1 | Wang et al. (2023a) | 27 | 20 | 15 | 10 |
| J2051−0827 | −46 | Han et al. (2018) | 13 | 7 | −1 | 8 |
| J2055+3829 | −65.8 | Wang et al. (2023a) | 17 | 17 | > 0.1 | > 0.1 |
| J2115+5448 | / | / | / | / | −3 | 4 |
| J2214+3000 | −44.5 | O’Sullivan et al. (2023) | 29 | 29 | > 0.1 | > 0.1 |
| J2234+0944 | −10.4 | Wang et al. (2023a) | 15 | 12 | 4 | 4 |
| J2256−1024 | 15.0 | Crowter et al. (2020) | 18 | 13 | 2 | 10 |
Notes. Rotation Measure (RM) values were taken from the articles listed in the “RM Reference” column. Polarised intensities (Ip), linear (⟨L⟩), circular (⟨V⟩) and absolute circular (⟨∥V∥⟩) intensities are quoted in percentages of the total intensity (I). See Sect. 4 for details on the analysis.
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