Table 2.
Days of observation around the 2024 April 29 Vela glitch.
| Date | Antenna | Duration [h] | epoch MJD | # pulses | Pobs [ms] | SNR |
|---|---|---|---|---|---|---|
| April 17 | A2 | 3.66 | 60417.86861037355 | 147394 | 89.42592924 | 348.18 |
| April 18 | A2 | 3.66 | 60418.86988352169 | 147394 | 89.42598438 | 274.62 |
| April 19 | A2 | 3.66 | 60419.86687426244 | 147363 | 89.42603628 | 263.84 |
| April 20 | A2 | 3.66 | 60420.61084910590 | 147389 | 89.42608723 | 261.88 |
| April 28 | A2 | 3.60 | 60428.34752565132 | 144793 | 89.42645908 | 219.39 |
| May 1 | A2 | 3.60 | 60431.83923799470 | 144791 | 89.42636648 | 276.11 |
| May 2 | A2 | 3.66 | 6043283136500318 | 147394 | 89.42640220 | 256.08 |
| May 3 | A2 | 3.66 | 60433.82876083651 | 147393 | 89.42643953 | 326.08 |
| May 4 | A2 | 3.53 | 60434.82621454021 | 142092 | 89.42647504 | 300.34 |
Notes. Date of each observation with A2, duration in hours, the MJD at the topocentric beginning of the observations, the corresponding number of single pulses analysed, instantaneous topocentric period, Pobs, and estimated signal to noise ratio (SNR) for the selected observations around the 2024 Vela glitch used for the pulse-by-pulse analysis. The estimated time of the glitch on April 29 is MJD 60429.8696.
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