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Table 4.
Nulling periodicity and intensity variations of ten pulsars.
| JName | Null freq. |
 |
 |
|---|---|---|---|
| (1/P) | |||
| J0304+1932 | 0.011 | 1.16 | 0.74 |
| J1136+1551 | – | 1.52 | 1.17 |
| J1239+2453 | – | 0.96 | 0.90 |
| J1509+5531 | 0.043 | 1.64 | 0.67 |
| J1709−1640 ( ‡ ) | 0.005 | 1.73 | 0.71 |
| J1932+1059 | – | 1.36 | 0.78 |
| J2022+5154 | – | 1.18 | 0.78 |
| J2048−1616 | – | 1.18 | 0.96 |
| J2313+4253 | 0.022 | 1.03 | 0.94 |
| J2321+6024 | – | 1.28 | 0.86 |
Notes. ( ‡ )Analysis is for the block-A data from 27 Oct 2017. ⟨I1⟩, ⟨I2⟩, ⟨I−1⟩, and ⟨I−2⟩, mean intensities of the first, the second, the last and the one but last subintegrations of emission.
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