Table A.1.
MUSE spectroscopic redshift catalogue.
ID | IDMUSE | R.A. | Dec | z | QF |
---|---|---|---|---|---|
(J2000) | (J2000) | ||||
– | 9900008 | 24.5229109 | −21.9260049 | 0.2789 | 9 |
– | 555552 | 24.5159631 | −21.9300671 | 0.3092 | 3 |
117 | 1738 | 24.5204485 | −21.9197347 | 0.3285 | 3 |
– | 1716* | 24.5232187 | −21.9209395 | 0.3291 | 3 |
320 | 1162 | 24.5178425 | −21.9303273 | 0.3307 | 2 |
– | 10002 | 24.5161968 | −21.9247577 | 0.3307 | 3 |
– | 10001 | 24.5172345 | −21.9235510 | 0.3311 | 3 |
78 | 1127 | 24.5149459 | −21.9276509 | 0.3316 | 3 |
– | 1619* | 24.5175558 | −21.9223099 | 0.3317 | 3 |
– | 555559* | 24.5171543 | −21.9208968 | 0.3318 | 3 |
– | 1686* | 24.5148629 | −21.9213703 | 0.3318 | 3 |
103 | 1073 | 24.512084 | −21.9252872 | 0.3323 | 3 |
– | 1644* | 24.516643 | −21.9222194 | 0.3324 | 3 |
261 | 5555521 | 24.5097565 | −21.9302674 | 0.3328 | 3 |
154 | 1498 | 24.5129692 | −21.9203716 | 0.3329 | 3 |
262 | 1218 | 24.5130061 | −21.9278434 | 0.3331 | 3 |
92 | 1304 | 24.5123572 | −21.9253942 | 0.3332 | 3 |
199 | 1782 | 24.5099978 | −21.9190911 | 0.3335 | 3 |
60 | 997 | 24.5153411 | −21.9329004 | 0.3336 | 2 |
115 | 1308 | 24.5114284 | −21.9213096 | 0.3337 | 3 |
76 | 1149 | 24.5228962 | −21.9298747 | 0.3338 | 3 |
– | 774 | 24.5099894 | −21.9291747 | 0.3339 | 3 |
142 | 1551 | 24.5143184 | −21.9224156 | 0.3341 | 3 |
– | 1316* | 24.5090635 | −21.9274273 | 0.3345 | 3 |
– | 1318* | 24.5089117 | −21.9274546 | 0.3348 | 3 |
70 | 1094 | 24.5119004 | −21.930871 | 0.3352 | 3 |
55 | 895 | 24.5162254 | −21.9326011 | 0.3353 | 3 |
85 | 1256 | 24.510652 | −21.9279027 | 0.3357 | 3 |
113 | 1475 | 24.5150361 | −21.9242069 | 0.3360 | 2 |
135 | 1535 | 24.5133605 | −21.9225114 | 0.3360 | 3 |
485 | 2000 | 24.51663 | −21.9244886 | 0.3363 | 3 |
129 | 1513 | 24.5201735 | −21.9229667 | 0.3365 | 3 |
93 | 555553 | 24.5141805 | −21.927675 | 0.3368 | 2 |
267 | 1642 | 24.5128585 | −21.9217549 | 0.3370 | 2 |
116 | 1457 | 24.5156388 | −21.9227696 | 0.3372 | 3 |
90 | 1211 | 24.5076178 | −21.9271544 | 0.3372 | 3 |
105 | 555554 | 24.5108496 | −21.9255751 | 0.3374 | 3 |
102 | 1210 | 24.5213768 | −21.9239768 | 0.3379 | 3 |
153 | 1630 | 24.5241351 | −21.919833 | 0.3379 | 3 |
106 | 5555536 | 24.5119913 | −21.9254078 | 0.3380 | 3 |
0 | 827 | 24.5157373 | −21.9254784 | 0.3381 | 3 |
58 | 930 | 24.5078679 | −21.9329074 | 0.3383 | 3 |
63 | 1049 | 24.5207142 | −21.9319295 | 0.3383 | 3 |
72 | 1147 | 24.5113797 | −21.9300727 | 0.3385 | 3 |
193 | 1631 | 24.5153499 | −21.9192529 | 0.3386 | 3 |
191 | 1386 | 24.5214401 | −21.9183725 | 0.3386 | 3 |
265 | 1783 | 24.5222923 | −21.9191665 | 0.3387 | 2 |
77 | 555551 | 24.5177768 | −21.9292971 | 0.3390 | 3 |
69 | 1032 | 24.5090052 | −21.9312181 | 0.3392 | 3 |
264 | 1582 | 24.5244402 | −21.9220557 | 0.3394 | 2 |
156 | 1633 | 24.5162417 | −21.9200615 | 0.3399 | 3 |
65 | 1003 | 24.5059888 | −21.9311714 | 0.3406 | 3 |
52 | 898 | 24.5257606 | −21.932203 | 0.3416 | 3 |
192 | 1701 | 24.5186628 | −21.9198871 | 0.3427 | 3 |
202 | 1549 | 24.5233304 | −21.9219431 | 0.3431 | 3 |
203 | 1433 | 24.516425 | −21.9212544 | 0.3436 | 3 |
– | 1431* | 24.5084096 | −21.9253918 | 0.3437 | 3 |
263 | 1543 | 24.5188906 | −21.9228596 | 0.3453 | 3 |
266 | 1595 | 24.515279 | −21.9220368 | 0.3463 | 3 |
189 | 1869 | 24.5140145 | −21.917715 | 0.3472 | 3 |
– | 1952 | 24.5166145 | −21.9171875 | 0.354 | 9 |
67 | 1066 | 24.5171971 | −21.9320865 | 0.370 | 3 |
82 | 873 | 24.5136363 | −21.9244078 | 0.371 | 3 |
51 | 751 | 24.5201843 | −21.932538 | 0.372 | 3 |
– | 1070 | 24.5127061 | −21.9320308 | 0.372 | 3 |
194 | 1608 | 24.5244187 | −21.9196872 | 0.376 | 3 |
– | 5555516 | 24.5132654 | −21.9305945 | 0.459 | 3 |
– | 9900014 | 24.5246215 | −21.9324916 | 0.522 | 3 |
– | 1838 | 24.5099019 | −21.9183388 | 0.541 | 3 |
– | 1911 | 24.5084136 | −21.9176089 | 0.602 | 3 |
– | 9900011 | 24.5103473 | −21.9294554 | 0.652 | 3 |
– | 1532 | 24.5150086 | −21.923182 | 0.767 | 3 |
– | 9900015 | 24.5146393 | −21.9262452 | 0.767 | 3 |
– | 1299 | 24.518391 | −21.9264267 | 0.767 | 3 |
187 | 1674 | 24.5103495 | −21.9164811 | 0.791 | 3 |
– | 1826 | 24.5088558 | −21.9189801 | 0.793 | 3 |
– | 1897 | 24.5075894 | −21.9178839 | 0.830 | 3 |
84 | 1200 | 24.5076133 | −21.9264195 | 0.830 | 3 |
– | 1436 | 24.50895 | −21.9250223 | 0.862 | 3 |
– | 1915 | 24.5085166 | −21.9174518 | 0.870 | 3 |
– | 1863 | 24.5163104 | −21.9182446 | 0.951 | 3 |
183 | 1917 | 24.5205768 | −21.9161932 | 0.952 | 3 |
– | 1117 | 24.5133754 | −21.931416 | 1.024 | 3 |
319 | 1093 | 24.5128482 | −21.931183 | 1.024 | 3 |
– | 1026 | 24.5189773 | −21.9332474 | 1.347 | 3 |
– | 1005 | 24.5188692 | −21.9332751 | 1.347 | 3 |
205 | 1683 | 24.508369 | −21.9205608 | 1.666 | 3 |
97 | 1332 | 24.5228653 | −21.9262572 | 1.759 | 3 |
– | 1755 | 24.5153988 | −21.9187909 | 1.945 | 2 |
– | 555558 | 24.5176138 | −21.9233427 | 1.949 | 3 |
– | 927 | 24.5132561 | −21.9299314 | 1.949 | 3 |
– | 364 | 24.5160096 | −21.9303706 | 1.949 | 3 |
– | 761 | 24.5099201 | −21.9260449 | 1.949 | 3 |
– | 1366 | 24.5255739 | −21.9265684 | 2.950 | 2 |
– | 9900003 | 24.5168229 | −21.9256552 | 3.152 | 3 |
– | 9900002 | 24.5180612 | −21.9255557 | 3.152 | 3 |
– | 9900004 | 24.5082954 | −21.9228268 | 3.152 | 3 |
– | 9900001 | 24.5209073 | −21.9318334 | 3.361 | 9 |
– | 9900005 | 24.507886 | −21.9242017 | 3.420 | 3 |
– | 9900006 | 24.5174131 | −21.9250015 | 3.420 | 3 |
– | 9900007 | 24.5158357 | −21.9247664 | 3.420 | 2 |
– | 9900009 | 24.5241269 | −21.9286028 | 3.584 | 9 |
– | 9900010 | 24.5226685 | −21.9224566 | 3.620 | 3 |
– | 9900012 | 24.5118702 | −21.9177915 | 4.068 | 3 |
– | 1175 | 24.5237221 | −21.9302823 | 4.354 | 2 |
– | 9900013 | 24.5238134 | −21.9247531 | 4.641 | 3 |
– | 1947 | 24.5175665 | -21.9173905 | 6.353 | 3 |
Notes. We identify the sources included in this catalogue with their photometric ID (see Ertl et al. 2025) and IDMUSE. We report the right ascension, declination, spectroscopic redshift z, and the corresponding uncertainty in terms of a QF, with 3 as secure, 2 as likely, and 9 as secure (based on a single emission line). The horizontal line separates objects at the cluster redshift from line-of-sight foreground and background galaxies. We mark the 13 lensed multiple images with a reliable redshift measurements (i.e. QF≥2) included in this catalogue with a bold-face ID, and the objects belonging to the cluster which are not galaxies with an asterisk (such non-galaxy objects are e.g. star-forming clumps of jellyfish galaxies at the cluster redshift). They have been excluded from the cluster member sample used by Ertl et al. (2025), Acebron et al. (2025), and Suyu et al. (in prep.) to build SL models of the cluster.
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