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Table A.1

Information on spectroscopically identified multiple images in MACS 1206.

ID RA Dec zMUSE μtot μtan/μrad Comments

1a 181.550916 8.797422 1.0121 HST/F606W
1b 181.549604 8.799294 1.0121 HST/F606W
1c 181.548870 8.806655 1.0121 HST/F606W

2a 181.546790 8.795680 1.0369 1.0348 HST/F105W
2b 181.544819 8.799553 1.0369 1.0336 HST/F105W
2c 181.545102 8.803052 1.0369 1.0336 HST/F105W

3a 181.550570 8.795568 1.0433 HST/F606W
3b 181.547611 8.799811 1.0433 HST/F606W
3c 181.548607 8.805281 1.0433 HST/F606W

4a 181.552987 8.794699 1.4248 MUSE
4b 181.548830 8.800057 1.4248 MUSE
4c 181.549752 8.807965 1.4248 MUSE
(4c) 181.554126 8.801587 blended with gal.

5a 181.553557 8.795189 1.4254 HST/F110W
5b 181.554237 8.801552 1.4254 HST/F110W
5c 181.550005 8.808098 1.4254 HST/F110W

6a 181.549979 8.796362 1.4255 HST/F606W
6b 181.548139 8.797058 1.4255 2.1743b HST/F606W
6c 181.548050 8.809283 1.4255 HST/F606W

7a 181.550563 8.795704 1.4257 HST/F606W
7b 181.547193 8.797998 1.4257 HST/F606W
7c 181.551339 8.800328 1.4257 HST/F606W
7d 181.552213 8.800398 1.4257 HST/F606W
7e 181.548307 8.808856 1.4257 HST/F606W

8a 181.553657 8.795756 1.4864 HST/F110W
8b 181.554524 8.801104 1.4864 HST/F110W
8c 181.549957 8.808887 1.4864 HST/F110W

9a 181.546741 8.793144 1.9600 HST/F606W
9b 181.543273 8.797812 1.9600 HST/F606W
9c 181.544378 8.807486 1.9600 HST/F606W

10a 181.552450 8.795001 2.5393 2.5398 HST/F606W
10b 181.546604 8.797465 2.5393 HST/F606W
10c 181.550487 8.799957 HST/F606W
10d 181.554894 8.800160 HST/F606W
10e 181.548827 8.811813 HST/F606W

11a 181.562654 8.796672 3.0358 3.0363 HST/F606W
11b 181.562495 8.804911 3.0358 3.0371 HST/F606W
11c 181.560573 8.808988 3.0358 3.0372 HST/F606W

12a 181.548632 8.793717 3.3890 MUSE
12b 181.546121 8.795387 3.3890 MUSE
12c 181.553268 8.800197 3.3890 MUSE
(12d) 181.551478 8.800081 blended with gal., low μ
(12e) 181.547097 8.812472 outside MUSE FoV

13a 181.549416 8.801768 3.3961 MUSE
13b 181.547859 8.802115 3.3961 MUSE
13c 181.553770 8.804759 3.3961 MUSE
13d 181.551389 8.806864 3.3961 MUSE
(13e) 181.554500 8.788383 outside MUSE FoV

14a 181.566558 8.804480 3.7531 HST/F625W
14b 181.566475 8.804733 3.7531 HST/F625W
14c 181.566475 8.805147 3.7531 HST/F625W
14d 181.566275 8.806328 3.7531 HST/F625W
14e 181.565591 8.807690 3.7531 HST/F625W

15a 181.555962 8.791635 3.7611 HST/F606W
15b 181.557600 8.803056 3.7611 HST/F606W
15c 181.551748 8.810964 HST/F606W

16a 181.554584 8.791202 3.7617 MUSE
16b 181.546465 8.799671 3.7617 MUSE
16c 181.556520 8.802471 3.7617 MUSE
(16d) 181.550432 8.811056 MUSE edge

17a 181.556136 8.795620 3.8224 MUSE
17b 181.556958 8.799422 3.8224 MUSE
(17c) 181.547557 8.798385 low μ
(17d) 181.550041 8.813393 outside MUSE FoV

18a 181.555376 8.796714 4.0400 HST/F814W
18b 181.555927 8.798595 4.0400 HST/F814W
(18c) 181.549137 8.798385 blended with gal., low μ

19a 181.562084 8.794875 4.0520 HST/F814W
19b 181.561873 8.805239 4.0520 HST/F814W
19c 181.559788 8.809463 4.0520 HST/F814W

20a 181.547472 8.800476 4.0553 MUSE
20b 181.556839 8.803813 4.0553 MUSE
(20c) 181.555448 8.790286 MUSE edge
(20d) 181.551634 8.810099 MUSE edge

21a 181.543431 8.797674 4.0718 MUSE
21b 181.551462 8.800814 4.0718 MUSE
21c 181.552850 8.801115 4.0718 MUSE
21d 181.553430 8.801204 4.0718 MUSE
(21e) 181.550064 8.791270 outside MUSE FoV

22a 181.544328 8.791418 4.2913 HST/F105W
22b 181.540282 8.796562 4.2913 close to bkg. galaxy
22c 181.540884 8.806094 4.2913 HST/F105W

23a 181.563252 8.796893 4.7293 MUSE
23b 181.563537 8.803670 4.7293 MUSE
23c 181.559832 8.811526 4.7293 close to bkg. galaxy

24a 181.551378 8.791300 5.6984 HST/F105W
24b 181.544085 8.797094 5.6984 HST/F105W
24c 181.550911 8.800607 5.6984 MUSE
24d 181.555210 8.801066 5.6984 HST/F105W
24e 181.546977 8.812247 5.7030 close to bkg. galaxy

25a 181.559714 8.796562 5.7927 MUSE
25b 181.560102 8.800177 5.7927 MUSE
(25c) 181.553429 8.813652 outside MUSE FoV

26a 181.550711 8.803112 6.0106 MUSE
26b 181.551211 8.803668 6.0106 MUSE
(26c) 181.553742 8.786102 outside MUSE FoV

27a 181.553251 8.798825 6.0601 MUSE
27b 181.551691 8.799167 6.0601 MUSE
(27c) 181.546863 8.814885 outside MUSE FoV

Notes. The magnification values, and their 68% confidence level errors, are computed using the reference model P3ε. IDs in brackets are model predicted multiple images with no identification in the MUSE and HST data, therefore not used in the modeling.

(*)

Multiple images nearby background galaxies that are not used in the strong lensing models.

(a)

Spectroscopic redshifts from CLASH-VLT with VIMOS (Zitrin et al. 2012).

(b)

The redshift of the multiple image 6b is reported with quality flag 2, i.e. reliability of 80%, in the public catalogue by Biviano et al. (2013).

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