Open Access

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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