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Table 1.

Catalog of the multiple images used as model constraints.

ID RA Dec zMUSE
1a 8.8537162 −20.2543192 5.0884
1b 8.8517093 −20.2565301 5.0884
1c 8.8486255 −20.2643074

2a 8.8571221 −20.2570308 2.0684
2b 8.8560776 −20.2581430 2.0684
2c 8.8523183 −20.2667410

3a 8.8583246 −20.2575877 1.2414
3b 8.8561510 −20.2597292 1.2414
3c 8.8539187 −20.2654209 1.2414

4a 8.8617091 −20.2535710
4b 8.8549683 −20.2619971 4.0124
4c 8.8544628 −20.2648364 4.0124

5a 8.8630883 −20.2580666 1.2787
5b 8.8609660 −20.2639830 1.2787
5c 8.8583770 −20.2665377 1.2787

6a 8.8624054 −20.2574650 4.1516
6b 8.8614047 −20.2625693 4.1516
6c 8.8552742 −20.2698532 4.1516

7a 8.8563501 −20.2573314 1.4506
7b 8.8558723 −20.2579503 1.4506
7c 8.8523546 −20.2652017 1.4506

Notes. IDs, coordinates (RA and Dec based on the RELICS public images) and redshifts (zMUSE) used as inputs to our lens model. Image 2c is too faint for a secure spectroscopic confirmation, and images 4a and 1c are located outside the MUSE field of view.

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