Table 4
Drift analysis results for three pulsars.
| P3 | P2 | m | ||||
| Pulsar |
|
|||||
| [P0] | [deg] | 21 cm | 92 cm | 192 cm | ||
|
|
||||||
| B1112+50... | 6 ± 3 |
|
1.5 | 2.1 | 3.5 | |
| B1133+16a... | 30 ± 5 | − | 1.4 | 0.8 | 2.2 | |
|
− | |||||
| B0031−07b... |
|
|
1.2 | 1.4 | 3.1 | |
| 6.7 ± 0.1 |
|
|||||
Notes. Vertical and horizontal separations of the subpulses are listed in Cols. 2 and 3, respectively. The value of modulation index m is the minimum in the longitude-resolved modulation index and is shown for three different wavelengths in the last three columns. The values in Col. 4 are from Weltevrede et al. (2006a), values in Col. 5 from Weltevrede et al. (2007), and the results in the last column are from this work.
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