Table B.2.
Multiple images used for strong lens mass modeling.
| ID | RA(J2000) | Dec(J2000) | Redshift | Ref.a |
|---|---|---|---|---|
| 1.1 | 93.967707 | −57.780612 | 1.358 | 1,2 |
| 1.2 | 93.966248 | −57.779779 | ||
| 1.3 | 93.962831 | −57.779168 | ||
| 2.1 | 93.967415 | −57.780807 | 1.358 | 1,2 |
| 2.2 | 93.966082 | −57.780001 | ||
| 2.3 | 93.962582 | −57.779334 | ||
| 2.4 | 93.965665 | −57.780529 | ||
| 3.1 | 93.967498 | −57.780918 | 1.358 | 1,2 |
| 3.2 | 93.965915 | −57.780029 | ||
| 3.3 | 93.962624 | −57.779445 | ||
| 3.4 | 93.965623 | −57.780584 | ||
| 4.1 | 93.967248 | −57.781140 | 1.358 | 1,2 |
| 4.2 | 93.962528 | −57.779634 | ||
| 4.3 | 93.965373 | −57.780945 | ||
| 5.1 | 93.955832 | −57.781418 | 1,2 | |
| 5.2 | 93.957207 | −57.782612 | ||
| 6.1 | 93.958303 | −57.781589 | 4.013 | 1,2 |
| 6.2 | 93.955874 | −57.776168 | ||
| 6.3 | 93.965873 | −57.776112 | ||
| 6.4 | 93.966582 | −57.774862 | ||
| 6.5 | 93.964284 | −57.779477 | ||
| 7.1 | 93.958837 | −57.779130 | 1.7 ± 0.5 | 3,4 |
| 7.2 | 93.964036 | −57.782170 | ||
| 7.3 | 93.970302 | −57.782715 | ||
| 8.1 | 93.965173 | −57.777030 | 1.8 ± 0.5 | 3,4 |
| 8.2 | 93.963320 | −57.776747 | ||
| 9.1 | 93.979824 | −57.772476 | 9.625b | 1,2,3,4,5 |
| 9.2 | 93.979314 | −57.772182 | ||
| 9.3 | 93.950004 | −57.770225 | ||
| 10.1 | 93.979695 | −57.772393 | 9.625b | 1,2,3,4,5 |
| 10.2 | 93.979412 | −57.772235 | ||
| 10.3 | 93.950003 | −57.770225 | ||
| 11.1 | 93.978702 | −57.771832 | 9.625b | 1,2,3,4,5 |
| 11.2 | 93.980386 | −57.772834 | ||
| 12.1 | 93.973333 | −57.767401 | 6.102b | 3,4 |
| 12.2 | 93.981540 | −57.769895 | ||
| 12.3 | 93.964613 | −57.766720 | ||
| 13.1 | 93.973327 | −57.777517 | 6.4 ± 0.5 | 3,4 |
| 13.2 | 93.944498 | −57.774728 | ||
| 14.1 | 93.981011 | −57.776970 | 3.2 ± 0.5 | 3,4 |
| 14.2 | 93.970332 | −57.772476 | ||
| 14.3 | 93.957967 | −57.772538 | ||
| 15.1 | 93.969522 | −57.783962 | 5 | |
| 15.2 | 93.964478 | −57.783726 | ||
| 15.3 | 93.955549 | −57.778803 | ||
| 16.1 | 93.950320 | −57.779373 | 3.569b | 5 |
| 16.2 | 93.960220 | −57.786883 | ||
| 16.3 | 93.972837 | −57.787069 | ||
| 17.1 | 93.950000 | −57.775647 | 4.880b | 5 |
| 17.2 | 93.960709 | −57.786008 | ||
| 17.3 | 93.970043 | −57.774477 | ||
| 17.4 | 93.969428 | −57.775505 | ||
| 18.1 | 93.946965 | −57.781198 | 5.842b | 5 |
| 18.2 | 93.970939 | −57.789100 | ||
Notes. The redshifts without errors show spectroscopic redshifts, while those with errors correspond to photometric redshifts. Larger errors of 0.5 in photometric redshifts, compared to measurement errors, are used as Gaussian priors for redshifts in mass modeling with glafic. The Lenstool model assumed broad priors of [1.5–8] for all arcs. Arcs number 5.1, 5.2, 13.1, 13.2, and 17.4 were not used in the Lenstool model. Otherwise, the models employed the same constraints.
References for multiple images. 1 – Paterno-Mahler et al. (2018); 2 – Salmon et al. (2018); 3 – Adamo et al. (2024); 4 – Bradley et al. (2025); 5 – this paper.
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