Table 1
Summary of the phase-average linear polarisation measurements for pulsars detected in the optical.
| Pulsar | τ | P s | Ṗ s | Ė | B S | B LC | PD | References |
| (103 yr) | (s) | (10-13 s s-1) | (1038 erg cm-2 s-1) | (1012 G) | (105 G) | (%) | ||
|
|
||||||||
| B0531+21 | 1.24 | 0.033 | 4.22 | 4.6 | 3.78 | 9.80 | 5.2 ± 0.3 | (1) |
| 5.5 ± 0.1 | (2) | |||||||
| B0540−69 | 1.67 | 0.050 | 4.79 | 1.5 | 4.98 | 3.62 | 5.0 ± 2.0 | (3) |
| 16.0 ± 4.0 | (4) | |||||||
| ≈5.0 | (5) | |||||||
| B1509−58 | 1.56 | 0.151 | 15.3 | 0.17 | 15.40 | 0.42 | 10.4 | (5) |
| B0833−45 | 11.3 | 0.089 | 1.25 | 0.069 | 3.38 | 0.44 | 8.1 ± 0.7 | (6) |
| 9.4 ± 4 | (7) | |||||||
| 8.5 ± 0.8 | (5) | |||||||
| B0656+14 | 111 | 0.384 | 0.55 | 0.00038 | 4.66 | 0.007 | 11.9 ± 5.5 | this work |
Notes. For the Crab, a value of the polarisation was obtained from phase-resolved observations by Słowikowska et al. (2009; 2012).
Reference. (1) Moran et al. (2013); (2) Słowikowska et al. (2012); (3) Lundqvist et al. (2011); (4) Mignani et al. (2010); (5) Wagner & Seifert (2000); (6) Moran et al. (2014); (7) Mignani et al. (2007).
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