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Table 1.

Overview of observed RGB stars in the MUSE survey for the 25 GCs investigated in this paper.

NGC Name RGB Valid V − VHB <  0.2
(1) (2) (3) (4) (5)
104 47 Tuc 2587 2538 354 (13.9%)
362 1236 1144 237 (20.7%)
1851 1454 1358 273 (20.1%)
1904 454 430
2808 2788 2512 713 (28.4%)
3201 139 137 41 (29.9%)
5139 ω Cen 1485 1421
5286 1376 1153 212 (18.4%)
5904 M 5 937 870 198 (22.8%)
6093 1315 1071 248 (23.2%)
6218 M 12 245 236
6254 M 10 439 399 90 (22.6%)
6266 M 62 2314 2191
6293 230 168
6388 4668 4098 741 (18.1%)
6441 4978 4408 1047 (23.8%)
6522 536 481
6541 910 820 135 (16.5%)
6624 581 539 72 (13.4%)
6656 M 22 423 397 83 (20.9%)
6681 M 70 344 327 71 (21.7%)
6752 578 539 82 (15.2%)
7078 M 15 1685 1318 337 (25.6%)
7089 M 2 1908 1727 377 (21.8%)
7099 M 30 341 290 71 (24.5%)

Total 33951 30572 5382 (17.6%)

Notes. (1) NGC number. (2) Alternative identifier (if any). (3) Total number of observed RGB stars, (4) of which have valid EW measurements, (5) of which are brighter than the HB (percentage relative to Col. 4).

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