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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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