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Table 7

Results for the 42 star forming regions and OCs in the sample, indicating, for each cluster: all stars (both UVES and GIRAFFE) from the GES sample and the number of stars detected with measured EW(Li) values, the number of stars selected as candidate members, and Li-rich giant field contaminants.

Cluster iDR6 stars Members Li-rich giants
All With Li # %(All) %(with Li) # %(All)
NGC 6530 1983 1330 343 17.3 25.8 11 0.6
ρ Oph 311 297 44 13.8 14.5 2 0.6
Trumpler 14 1902 1056 159 8.4 15.1 11 0.6
Cha I 707 659 87 12.3 13.2 6 0.8
NGC 2244 452 391 116 25.7 29.7 1 0.2
NGC 2264 1853 1609 503 27.1 31.3 10 0.5
λ Ori 836 778 161 19.3 20.7 3 0.4
Col 197 409 366 92 22.5 25.1 7 1.7
γ Vel 1262 1190 234 18.5 19.7 1 0.1
NGC 2232 1869 1750 68 3.6 3.9 9 0.5
NGC 2547 477 405 151 31.7 37.3 0 0.0
IC 2391 434 400 35 8.1 8.8 6 1.4
IC 2602 1852 1740 55 3.0 3.2 24 1.3
IC 4665 567 544 33 5.8 6.1 0 0.0
NGC 2451 A/B 1656 1607 106 6.4 6.6 10 0.6

NGC 6405 701 498 51 7.3 10.2 1 0.1
Blanco 1 463 404 96 20.7 23.8 0 0.0
NGC 6067 780 343 56 7.2 16.3 0 0.0
NGC 6649 283 62 2 0.7 3.2 0 0.0
NGC 2516 759 677 376 49.5 55.5 0 0.0
NGC 6709 730 600 49 6.7 8.2 10 1.4
NGC 6259 494 278 35 7.1 12.6 0 0.0
NGC 6705 1066 610 139 13.0 22.8 0 0.0
Berkeley 30 332 157 24 7.2 15.3 0 0.0
NGC 6281 320 221 23 7.2 10.4 1 0.3
NGC 3532 1145 860 384 33.5 44.7 11 1.0
NGC 4815 218 104 29 13.3 27.9 0 0.0
NGC 6633 1662 1501 67 4.0 4.5 9 0.5

NGC 2477 125 10 9 7.2 90.0 0 0.0
Trumpler 23 165 85 23 13.9 27.1 0 0.0
Berkeley 81 279 173 24 8.6 13.9 0 0.0
NGC 2355 208 160 86 41.4 53.8 0 0.0
NGC 6802 197 82 32 16.2 39.0 2 1.0
NGC 6005 560 317 49 8.8 15.5 3 0.5
Pismis 18 142 82 10 7.0 12.2 0 0.0
Melotte 71 120 9 4 3.4 44.5 0 0.0
Pismis 15 333 211 31 9.3 14.7 1 0.3
Trumpler 20 1213 430 104 8.6 24.2 0 0.0
Berkeley 44 93 80 30 32.3 37.5 0 0.0
NGC 2243 661 603 289 43.7 48.0 8 1.2
M67 131 121 96 73.3 79.3 0 0.0

Notes. Regarding member stars, we provide their percentages with respect to all GES stars and to those with a EW(Li) measurement in the field of each cluster.

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