Open Access
Table B.2.
Multiply imaged systems used as constraints in the MACS0257 mass model.
| ID | α (J2000) | δ (J2000) | zsystem |
|---|---|---|---|
| h m s | ° ′ ″ | ||
| 1.1 | 02:57:41.84 | −22:09:07.78 | 4.69 |
| 1.2 | 02:57:41.14 | −22:08:55.06 | 4.69 |
| 1.3 | 02:57:40.65 | −22:09:02.51 | 4.69 |
| 1.4 | 02:57:41.28 | −22:09:12.14 | 4.69 |
| 1.5 | 02:57:40.58 | −22:09:53.75 | 4.69 |
| 2.1 | 02:57:41.70 | −22:08:55.93 | 3.22 |
| 2.2 | 02:57:42.22 | −22:09:01.45 | 3.22 |
| 2.3 | 02:57:42.01 | −22:09:03.35 | 3.22 |
| 2.4 | 02:57:40.67 | −22:09:08.42 | 3.22 |
| 2.5 | 02:57:41.02 | −22:09:13.12 | 3.22 |
| 3.1 | 02:57:41.60 | −22:08:54.63 | 3.85 |
| 3.2 | 02:57:42.26 | −22:09:02.79 | 3.85 |
| 3.3 | 02:57:42.04 | −22:09:03.80 | 3.85 |
| 3.4 | 02:57:40.59 | −22:09:06.97 | 3.85 |
| 3.5 | 02:57:41.07 | −22:09:13.62 | 3.85 |
| 4.1 | 02:57:42.20 | −22:09:11.27 | 1.1690 |
| 4.2 | 02:57:41.66 | −22:08:58.31 | 1.1690 |
| 4.3 | 02:57:40.68 | −22:09:13.19 | 1.1690 |
| 4.4 | 02:57:41.35 | −22:09:40.82 | 1.1690 |
| 5.1 | 02:57:41.93 | −22:08:52.85 | 6.609 |
| 5.2 | 02:57:41.00 | −22:09:13.89 | 6.609 |
| 5.3 | 02:57:42.56 | −22:09:02.04 | 6.609 |
| 5.4 | 02:57:40.51 | −22:09:08.11 | 6.609 |
| 6.1 | 02:57:40.63 | −22:09:27.31 | 2.424 |
| 6.2 | 02:57:40.94 | −22:09:21.98 | 2.424 |
| 6.3 | 02:57:41.70 | −22:08:37.86 | 2.424 |
| 7.1 | 02:57:39.43 | −22:09:25.85 | 4.69 |
| 7.2 | 02:57:39.97 | −22:09:35.87 | 4.69 |
| 8.1 | 02:57:39.12 | −22:09:23.93 | 6.080 |
| 8.2 | 02:57:39.80 | −22:09:38.90 | 6.080 |
| 8.3 | 02:57:42.10 | −22:09:21.02 | 6.080 |
| 9.1 | 02:57:42.54 | −22:09:34.09 | 1.157 |
| 9.2 | 02:57:42.96 | −22:09:16.84 | 1.157 |
| 9.3 | 02:57:42.75 | −22:09:04.58 | 1.157 |
| 10.1 | 02:57:40.08 | −22:09:18.37 | 1.169 |
| 10.2 | 02:57:41.91 | −22:09:23.23 | 1.169 |
| 10.3 | 02:57:41.36 | −22:08:50.94 | 1.169 |
| 11.1 | 02:57:40.00 | −22:09:39.21 | 3.01 |
| 11.2 | 02:57:41.99 | −22:09:19.72 | 3.01 |
| 11.3 | 02:57:39.17 | −22:09:17.02 | 3.01 |
| 12.1 | 02:57:39.43 | −22:09:13.13 | 3.807 |
| 12.2 | 02:57:40.72 | −22:09:44.42 | 3.807 |
| 12.3 | 02:57:42.59 | −22:09:20.14 | 3.807 |
| 13.1 | 02:57:41.42 | −22:09:25.43 | 3.9545 |
| 13.2 | 02:57:41.77 | −22:09:31.50 | 3.9545 |
| 14.1 | 02:57:42.33 | −22:09:18.32 | 4.030 |
| 14.2 | 02:57:40.31 | −22:09:44.13 | 4.030 |
| 14.3 | 02:57:39.22 | −22:09:09.52 | 4.030 |
| 15.1 | 02:57:39.72 | −22:09:01.01 | 6.467 |
| 15.2 | 02:57:42.73 | −22:09:12.33 | 6.467 |
| 16.1 | 02:57:41.50 | −22:09:44.09 | 6.225 |
| 16.2 | 02:57:39.60 | −22:09:19.20 | 6.225 |
| 16.3 | 02:57:42.78 | −22:09:25.64 | 6.225 |
| 17.1 | 02:57:43.16 | −22:09:28.32 | 6.066 |
| 17.2 | 02:57:40.19 | −22:09:16.17 | 6.066 |
| 17.3 | 02:57:42.50 | −22:09:43.96 | 6.066 |
| 18.1 | 02:57:41.57 | −22:09:18.13 | 5.277 |
| 18.2 | 02:57:41.72 | −22:09:18.32 | 5.277 |
| 18.3 | 02:57:39.69 | −22:09:40.47 | 5.277 |
| 18.4 | 02:57:38.87 | −22:09:11.93 | 5.277 |
| 19.1 | 02:57:40.08 | −22:09:16.65 | 3.223 |
| 19.2 | 02:57:42.18 | −22:09:41.76 | 3.223 |
| 19.3 | 02:57:42.88 | −22:09:26.79 | 3.223 |
| 20.1 | 02:57:40.25 | −22:09:11.22 | 3.246 |
| 20.2 | 02:57:42.94 | −22:09:11.99 | 3.246 |
| 20.3 | 02:57:41.91 | −22:09:48.63 | 3.246 |
| 20.4 | 02:57:41.99 | −22:08:49.57 | 3.246 |
| 21.1 | 02:57:41.54 | −22:08:50.35 | 4.685 |
| 21.2 | 02:57:40.01 | −22:08:58.30 | 4.685 |
| 21.3 | 02:57:42.54 | −22:09:09.24 | 4.685 |
| 22.1 | 02:57:40.42 | −22:09:10.47 | 5.32295 |
| 22.2 | 02:57:42.90 | −22:09:06.61 | 5.32295 |
| 22.3 | 02:57:42.14 | −22:08:51.40 | 5.32295 |
| 23.1 | 02:57:41.33 | −22:09:27.77 | 5.557 |
| 23.2 | 02:57:41.41 | −22:09:32.43 | 5.557 |
| 24.1 | 02:57:39.17 | −22:09:16.02 | 4.69 |
| 24.2 | 02:57:42.37 | −22:09:20.51 | 4.69 |
| 24.3 | 02:57:40.25 | −22:09:42.65 | 4.69 |
| 24.4 | 02:57:41.07 | −22:08:42.03 | 4.69 |
| 25.1 | 02:57:42.07 | −22:09:26.07 | 4.4633 |
| 25.2 | 02:57:41.26 | −22:09:20.27 | 4.4633 |
Notes. From left to right: identification number for the multiple image, sky coordinates, redshift constraints from spectroscopy. Redshifts with error bars are not constrained with spectroscopy and are predictions from our lens model.
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