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Table 2.

Observations of Sgr A* used in this work, taken during the 2017 GMVA campaign.

Scan Start time (UTC) End time (UTC)
No0133 2017-04-03 07:46:05 2017-04-03 07:53:05
No0134 2017-04-03 07:55:05 2017-04-03 08:02:05
No0142 2017-04-03 08:16:13 2017-04-03 08:23:13
No0143 2017-04-03 08:25:13 2017-04-03 08:32:13
No0152 2017-04-03 08:46:22 2017-04-03 08:53:22
No0153 2017-04-03 08:55:22 2017-04-03 09:02:22
No0217 2017-04-03 12:17:08 2017-04-03 12:24:08
No0220 2017-04-03 12:26:08 2017-04-03 12:33:08
No0227 2017-04-03 12:47:05 2017-04-03 12:54:05
No0230 2017-04-03 12:56:05 2017-04-03 13:03:05
No0237 2017-04-03 13:17:01 2017-04-03 13:24:01
No0240 2017-04-03 13:26:01 2017-04-03 13:33:01
No0242 2017-04-03 13:38:31 2017-04-03 13:45:31
No0243 2017-04-03 13:47:01 2017-04-03 13:54:01
No0250 2017-04-03 14:12:01 2017-04-03 14:19:01
No0252 2017-04-03 14:24:31 2017-04-03 14:31:31
No0253 2017-04-03 14:33:01 2017-04-03 14:40:01

Notes. The data is centered at 86.268 GHz with 2 GHz of bandwidth. Each scan consists of multiple PSRFITS files containing full Stokes information.

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