Table 2
Details of the 8-hour observations.
| LOFAR SAS ID | Start Date and Time (UTC) | Phase |
|---|---|---|
| L776013 | 2020-04-14 20:00 | 0.73–0.83 |
| L776035(a) | 2020-04-15 20:00 | 0.93–0.03 |
| L779351 | 2020-04-23 19:30 | 0.34–0.44 |
| L779361 | 2020-04-24 19:00 | 0.64–0.74 |
| L780101 | 2020-04-28 19:00 | 0.85–0.95 |
| L780111 | 2020-04-29 19:00 | 0.15–0.25 |
| L780121 | 2020-05-01 18:30 | 0.75–0.85 |
| L780131 | 2020-05-02 18:30 | 0.05–0.15 |
Notes. Similar to Turner et al. (2021), we calculate the orbital phases relative to the periastron, where the planet’s orbital period is 3.31 days and the periastron time is 2446957.81JD (Wang & Ford 2011). (a)This dataset could not be properly calibrated due to intense ionospheric phase and amplitude scintillations.
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