Table 1.
Properties of the NRT dataset used in this study.
| Pulsar | Time span (d) | Nobs | Median S/N |
|---|---|---|---|
| J0023+0923 | 4487 | 688 | 27.0 |
| J0610−2100 | 4527 | 211 | 40.1 |
| J0636+5128 | 3677 | 416 | 55.6 |
| J1124−3653 | 4447 | 348 | 6.5 |
| J1513−2550 | 3594 | 207 | 27.0 |
| J1544+4937 | 3953 | 67 | 15.8 |
| J1555−2908 | 833 | 79 | 20.6 |
| J1628−3205 | 3962 | 145 | 29.5 |
| J1705−1903 | 439 | 69 | 141.7 |
| J1719−1438 | 4519 | 30 | 31.1 |
| J1731−1847 | 4504 | 52 | 26.8 |
| J1745+1017 | 4503 | 43 | 38.9 |
| J1959+2048 | 4460 | 125 | 15.4 |
| J2051−0827 | 4520 | 181 | 96.3 |
| J2055+3829 | 2989 | 523 | 17.7 |
| J2115+5448 | 3162 | 143 | 28.9 |
| J2214+3000 | 4493 | 168 | 21.5 |
| J2234+0944 | 4523 | 303 | 55.0 |
| J2256−1024 | 1854 | 217 | 52.4 |
Notes. For each pulsar, we list the total time span of the observations, the number of observations, and the median signal-to-noise ratio (S/N) of the frequency- and time-averaged observations. In this study we considered all available NRT observations recorded using the NUPPI backend until MJD 60369 (29 February 2024).
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