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Table A.1.

Coordinates, redshifts, and magnification estimates of the 62 multiple images used to build the lens model of PSZ1-G311.

ID RA Dec z μ
2.1a 15:50:17.10 -78:11:42.3 *
2.1b 15:50:00.34 -78:11:25.3 *

2.2a 15:50:17.29 -78:11:40.8 *
2.2b 15:50:00.33 -78:11:26.3 *

3a 15:50:16.12 -78:11:41.7 2.393
3b 15:49:58.86 -78:11:33.6 2.393

4a 15:50:14.23 -78:11:38.2 1.186
4b 15:50:02.16 -78:11:24.0 1.186
5.1a 15:50:07.40 -78:10:57.2 2.3702
5.1b 15:50:06.14 -78:10:58.1 2.3702
5.1c 15:50:05.98 -78:10:58.3 2.3702
5.1d 15:50:04.59 -78:10:59.6 2.3702
5.1e 15:50:04.39 -78:10:59.9 2.3702
5.1f 15:50:04.20 -78:11:00.2 2.3702
5.1g 15:50:02.22 -78:11:04.9 2.3702
5.1h 15:50:00.37 -78:11:10.7 2.3702
5.1i 15:49:59.96 -78:11:12.4 2.3702
5.1l 15:49:59.75 -78:11:13.6 2.3702
5.1m 15:49:58.54 -78:11:26.9 2.3702
5.1n 15:50:15.09 -78:11:47.5 2.3702

5.2a 15:50:06.75 -78:10:57.5 2.3702
5.2b 15:50:06.59 -78:10:57.6 2.3702
5.2c 15:50:05.75 -78:10:58.6 2.3702
5.2d 15:50:04.84 -78:10:59.3 2.3702
5.2g 15:50:02.12 -78:11:05.2 2.3702
5.2h 15:50:00.92 -78:11:08.8 2.3702
5.2m 15:49:58.56 -78:11:27.1 2.3702
5.2n 15:50:15.18 -78:11:47.1 2.3702

5.3c 15:50:05.64 -78:10:58.7 2.3702
5.3d 15:50:04.98 -78:10:59.2 2.3702
5.3g 15:50:02.00 -78:11:05.6 2.3702
5.3h 15:50:01.19 -78:11:07.9 2.3702
5.3m 15:49:58.57 -78:11:27.3 2.3702
5.3n 15:50:15.24 -78:11:46.9 2.3702

5.4a 15:50:07.32 -78:10:57.3 2.3702
5.4b 15:50:06.23 -78:10:58.0 2.3702
5.4c 15:50:05.93 -78:10:58.4 2.3702
5.4d 15:50:04.64 -78:10:59.5 2.3702
5.4e 15:50:04.36 -78:10:59.9 2.3702
5.4f 15:50:04.23 -78:11:00.2 2.3702

5.5a 15:50:06.88 -78:10:57.4 2.3702
5.5b 15:50:06.52 -78:10:57.6 2.3702
5.5c 15:50:05.75 -78:10:58.5 2.3702
5.5d 15:50:04.81 -78:10:59.2 2.3702

5.6a 15:50:07.04 -78:10:57.1 2.3702
5.6b 15:50:06.50 -78:10:57.4 2.3702
5.6c 15:50:05.69 -78:10:58.4 2.3702
5.6d 15:50:04.82, -78:10:59.0 2.3702

5.7c 15:50:05.68 -78:10:58.8 2.3702
5.7d 15:50:04.97 -78:10:59.3 2.3702

5.8c 15:50:05.59 -78:10:58.7 2.3702
5.8d 15:50:05.05 -78:10:59.1 2.3702

5.9c 15:50:05.55 -78:10:58.6 2.3702
5.9d 15:50:05.06 -78:10:58.9 2.3702

5.11c 15:50:05.47 -78:10:58.7 2.3702
5.11d 15:50:05.17 -78:10:58.9 2.3702

5.12g 15:50:01.80 -78:11:05.8 2.3702
5.12h 15:50:01.44 -78:11:06.8 2.3702

5.13g 15:50:01.79 -78:11:06.4 2.3702
5.13h 15:50:01.55 -78:11:07.1 2.3702

5.14i 15:50:00.00 -78:11:12.6 2.3702
5.14l 15:49:59.80 -78:11:13.7 2.3702

Notes. The multiple images are grouped by families, separated by the horizontal black lines. The redshifts are measured from the MUSE spectra. The magnification values are estimated from the lens model. We report the median values obtained by sampling the model parameter posterior distribution functions to derive 100 realizations of the magnification maps. The quoted errors correspond to the 16th and 84th percentiles of the magnification distributions at each image position. (*) The redshifts of Sys-2 are estimated with LensTool (see Sect. 4.2).

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