Table 1.
MeerKAT observations of Ter5 used for this work.
| Observation id | Observation date | Start time | Length | Primary backend | tsamp | Npol | fc | BW | Nchan | Nant | Nbeam |
|---|---|---|---|---|---|---|---|---|---|---|---|
| (MJD) | (s) | (μs) | (MHz) | (MHz) | |||||||
| 01L ( † ) | 27 May 2019 | 58630.813 | 9000 | PTUSE | 9.57 | 4 | 1284 | 642 | 768 | 42 | 1 |
| 02L-orb ( † ) | 26 Feb 2020 | 58905.048 | 12 600 | PTUSE | 9.57 | 4 | 1284 | 856 | 4096 | 42 | 1 |
| 03L-orb ( † ) | 27 Feb 2020 | 58906.017 | 12 600 | PTUSE | 9.57 | 4 | 1284 | 856 | 4096 | 42 | 1 |
| 04L-orb ( † ) | 28 Feb 2020 | 58907.022 | 12 600 | PTUSE | 9.57 | 4 | 1284 | 856 | 4096 | 42 | 1 |
| 05L-orb ( † ) | 28 Feb 2020 | 58907.326 | 12 600 | PTUSE | 9.57 | 4 | 1284 | 856 | 4096 | 42 | 1 |
| 06L (*, 1) | 05 Sep 2020 | 59097.671 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 56 | 288 |
| 07L (*, 2) | 06 Jan 2021 | 59342.278 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 56 | 288 |
| 08L-orb ( * ) | 26 Jun 2023 | 59342.586 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 60 | 22 |
| 09L-orb ( * ) | 27 Jun 2023 | 59355.253 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 60 | 22 |
| 10L-orb ( * ) | 28 Jun 2023 | 59355.628 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 60 | 22 |
| 11L-orb ( * ) | 30 Jun 2023 | 59358.242 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 60 | 22 |
| 12L-orb ( * ) | 07 July 2023 | 59360.607 | 14 400 | APSUSE | 76.56 | 1 | 1284 | 856 | 4096 | 60 | 22 |
Notes. tsamp: sampling time; Npol: number of Stokes parameters; fc: central frequency; BW: observing bandwidth; Nchan: number of frequency channels; Nant: number of antennas; Nbeam: number of tied-array beams. The “-orb” in the Observation id indicates observations made as part of campaigns to derive orbital solutions for newly discovered pulsars. ( * )TRAPUM observations with single beam PTUSE data recorded in parallel. ( † )MeerTIME observations. (1)Refers to Epoch 1 and (2)to Epoch 2, respectively (see text).
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