Table A.2.
Observations of 47 Tuc made by the Parkes radio telescope with UWL frontend.
| Project / | Start date | Length | tsamp | DM |
|---|---|---|---|---|
| Proposal ID | and time (UTC) | (min) | (μs) | (pc cm−3) |
| P981 | 2018-11-16 12:39 | 60 | 64 | 24.6 |
| P982 | 2019-01-04 07:06 | 120 | 64 | 24.4 |
| P982 | 2019-01-04 09:08 | 120 | 64 | - |
| P982 | 2019-01-04 11:16 | 120 | 8 | 24.4 |
| P1006 | 2019-08-19 15:32 | 440 | 64 | 24.36 |
| P1022 | 2019-11-18 08:54 | 481 | 64 | 24.36 |
| P1022 | 2019-11-23 09:06 | 293 | 64 | 24.36 |
| P1022 | 2019-11-23 09:06 | 293 | 64 | 24.36 |
| P1022 | 2019-11-24 14:14 | 24 | 64 | 24.36 |
| P1022 | 2019-11-24 15:19 | 24 | 64 | 24.36 |
| P1022 | 2019-11-25 10:27 | 63 | 64 | 24.36 |
| P1022 | 2019-11-26 09:50 | 127 | 64 | 24.36 |
| P1022 | 2019-12-01 11:16 | 105 | 64 | 24.36 |
| P1022 | 2019-12-02 09:44 | 84 | 64 | 24.36 |
| P1022 | 2019-12-08 08:44 | 385 | 64 | 24.36 |
| P1022 | 2019-12-08 08:44 | 385 | 64 | 24.36 |
| P1022 | 2019-12-11 12:24 | 97 | 64 | 24.36 |
| P1022 | 2019-12-14 13:21 | 69 | 64 | 24.36 |
| P1022 | 2019-12-16 13:20 | 99 | 64 | 24.36 |
| P1022 | 2019-12-17 13:17 | 104 | 64 | 24.36 |
| P1022 | 2019-12-18 13:20 | 98 | 64 | 24.36 |
| P1022 | 2019-12-19 13:19 | 95 | 64 | 24.36 |
| P1022 | 2019-12-20 12:49 | 122 | 64 | 24.36 |
| P1054 | 2020-04-14 01:20 | 100 | 64 | 24.4 |
| PX061 | 2020-05-20 20:52 | 37 | 64 | - |
| P1076 | 2021-01-25 04:59 | 106 | 64 | 24.36 |
| P595 | 2022-09-07 10:01 | 90 | 64 | - |
| PX145 | 2025-12-17 08:16 | 223 | 64 | 24.4 |
Notes. tsamp is the sampling time and the DMs used for coherent dedispersion are listed in the last column. Pulsar 47 Tuc ai was not detected in any of these observations. The observation under P595 was done between 1344.5 to 1599.5 MHz frequency range and the rest have entire UWL bandwidth of 704 to 4032 MHz.
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