Table 3.
Correlation coefficients between Δνk and Δτk + 1.
| PSR name | Ng | rp | pp | rs | ps |
|---|---|---|---|---|---|
| J0205+6449 | 13 | 0.88 | 0.0002 | 0.76 | 0.004 |
| B0531+21 | 25 | −0.10 | 0.62 | −0.12 | 0.57 |
| J0537−6910 | 45 | 0.95 | 10−22 | 0.95 | 10−23 |
| J0631+1036 | 17 | 0.93 | 10−7 | 0.20 | 0.45 |
| B0833−45 | 20 | 0.24 | 0.31 | 0.31 | 0.21 |
| B1338−62 | 23 | 0.59 | 0.003 | 0.70 | 0.0002 |
| B1737−30 | 36 | 0.29 | 0.09 | 0.29 | 0.08 |
| B1758−23 | 13 | 0.76 | 0.003 | 0.80 | 0.001 |
Notes. The first and second columns contain the names of the pulsars and the respective number of glitches detected, respectively. The third and fourth columns correspond to the Pearson linear correlation coefficient rp and the respective p-value pp. The last two columns correspond to the Spearman correlation coefficient rs and the respective p-value ps.
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