Table D.1
Phase centres and integrated fluxes of the 24 systems analysed in ARKS derived from the primary beam corrected images.
| Name | Date [d/m/y] | RA [h:m:s] | Dec [d:m:s] | ΔRAg [mas] | ∆DecG [mas] | Wavelength [mm] | Flux [mJy] | Aperture size [au (″)] |
|---|---|---|---|---|---|---|---|---|
| HD 9672 | 17/06/2024 | 01:34:37.9394 | −15:40:34.967 | 1 | 0 | 0.89 | 13.9 ± 1.4 | 411 (7.2) |
| HD 10647 | 08/05/2024 | 01:42:29.7722 | −53:44:29.508 | 1 | 0 | 0.89 | 14.8 ± 1.5 | 197(11.3) |
| HD 14055 | 26/07/2024 | 02:17:18.9573 | +33:50:48.612 | 17 | 10 | 0.89 | 8.1 ± 0.9 | 333 (9.3) |
| HD 15115 | 09/05/2023 | 02:26:16.3839 | +06:17:32.012 | −1 | 1 | 0.89 | 4.8 ± 0.5 | 144 (2.9) |
| HD 15257 | 19/10/2022 | 02:28:09.9531 | +29:40:07.632 | −3 | −3 | 0.89 | 3.8 ± 0.5 | 352 (7.2) |
| HD 32297 | 23/09/2023 | 05:02:27.4455 | +07:27:39.119 | −1 | 2 | 0.89 | 10.8 ± 1.1 | 308 (2.4) |
| HD 39060 | 08/08/2015 | 05:47:17.0931 | −51:03:58.137 | 67 | 46 | 1.33 | 18.6 ± 1.9 | 194 (9.9) |
| HD 61005 | 11/05/2023 | 07:35:47.3591 | −32:12:12.298 | 0 | 1 | 0.89 | 14.8 ± 1.5 | 135 (3.7) |
| HD 76582 | 16/10/2022 | 08:57:35.2957 | +15:34:53.094 | 0 | 0 | 0.89 | 8.1 ± 0.9 | 489 (10.0) |
| HD 84870 | 24/12/2022 | 09:49:02.7913 | +34:05:06.134 | 0 | 0 | 0.89 | 2.6 ± 0.3 | 413 (4.7) |
| HD 92945 | 17/12/2016 | 10:43:27.9966 | −29:03:52.304 | −8 | 5 | 0.86 | 11.1 ± 1.1 | 156 (7.3) |
| HD 95086 | 09/01/2023 | 10:57:02.8496 | −68:40:02.161 | 0 | 0 | 0.89 | 9.3 ± 1.0 | 467 (5.4) |
| HD 107146 | 03/05/2021 | 12:19:06.2413 | +16:32:50.707 | −1 | −1 | 1.00 | 22.1 ± 2.2 | 182 (6.6) |
| HD 109573 | 04/06/2023 | 12:36:00.9175 | −39:52:10.778 | 0 | −1 | 0.89 | 13.8 ± 1.4 | 116 (1.6) |
| HD 121617 | 11/05/2023 | 13:57:41.0610 | −47:00:34.792 | 0 | 0 | 0.89 | 4.2 ± 0.4 | 157 (1.3) |
| HD 131488 | 27/06/2023 | 14:55:07.9902 | −41:07:13.925 | 0 | 0 | 0.89 | 7.4 ± 0.8 | 364 (2.4) |
| HD 131835 | 30/04/2023 | 14:56:54.4230 | −35:41:44.244 | 0 | 0 | 0.89 | 6.6 ± 0.7 | 298 (2.3) |
| HD 145560 | 19/05/2023 | 16:13:34.2891 | −45:49:04.446 | 0 | 0 | 0.89 | 4.6 ± 0.5 | 270 (2.2) |
| HD 161868 | 01/10/2022 | 17:47:53.5203 | +02:42:24.505 | 27 | 4 | 0.89 | 7.5 ± 0.8 | 283 (9.5) |
| HD 170773 | 23/01/2023 | 18:33:01.0908 | −39:53:33.111 | 0 | 0 | 0.89 | 14.2 ± 1.5 | 252 (6.8) |
| HD 197481 | 18/08/2014 | 20:45:09.8511 | −31:20:32.517 | 5 | −19 | 1.35 | 4.7 ± 0.5 | 52 (5.3) |
| HD 206893 | 30/08/2018 | 21:45:22.0239 | −12:47:00.064 | 15 | −6 | 1.35 | 1.0 ± 0.1 | 200 (4.9) |
| TYC 9340-437-1 | 02/10/2022 | 22:42:49.3897 | −71:42:22.415 | 0 | 0 | 0.89 | 9.5 ± 1.0 | 227 (6.2) |
| HD 218396 | 29/05/2018 | 23:07:28.8587 | +21:08:02.399 | 15 | −2 | 0.88 | 7.1 ± 0.8 | 412(10.1) |
Notes. Columns 2-6 display the date and the phase centre coordinates of the reference execution block in the ICRS frame used to align the observations during the correction step, and the offset relative to the predicted stellar position according to Gaia DR3 (the RA offset has been multiplied by cos(Dec), Gaia Collaboration 2023). Columns 7-9 show the wavelength, integrated flux, and aperture size. For systems with submillimetre galaxies, we used the subtracted images. The flux errors include a nominal 10% absolute flux calibration error added in quadrature to the statistical error that arises from the image rms. The aperture size corresponds to the semi-major axis of an elliptical mask used to measure the flux.
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