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Table 2

Gaia-ESO PMS analysis output parameters.

Parameter ρ Oph Cha I NGC 2264 γ Vel NGC 2547 NGC 6705

G U G U G U G U G U G U

raw

W(Hα) 25 5 87 14 387 24 203 2 106 1 0 0
W(Li) 189 23 633 47 1610 114 1186 75 404 25 708 48
Hα 10% 33 5 103 14 807 23 264 2 239 1 0 0

fundamental

Teff 170 21 572 39 1324 70 1104 51 361 24 394 32
log g 170 21 156 39 226 70 350 51 106 24 150 32
γ 156 ... 508 ... 1199 ... 1043 ... 337 ... 0 ...
[Fe/H] 170 21 515 39 1203 70 1018 51 311 24 360 32
ξ ... 14 ... 23 ... 42 ... 46 ... 15 ... 30
vsini 154 23 521 42 1192 83 1004 75 332 25 107 33
r 4 3 20 7 77 6 5 0 5 0 0 0

derived

log ϵ(Li) 154 23 514 40 1203 80 1017 57 311 25 356 31
log ϵ(X) ... 15 ... 28 ... 39 ... 46 ... 14 ... 31
acc 14 4 56 7 212 11 40 1 21 0 0 0
ΔW(Hα)chr 21 12 69 29 267 50 205 18 115 16 61 0
ΔW(Hβ)chr ... 10 ... 18 ... 42 ... 14 ... 12 ... 0
F(Hα)chr 21 12 65 28 265 47 199 17 105 16 47 0
F(Hβ)chr ... 10 ... 17 ... 41 ... 14 ... 12 ... 0

Notes. Columns 2–13 list the number of stars in each cluster for which the parameter was derived from GIRAFFE (G) and UVES (U) spectra separately in iDR2. Lithium parameters and vsini counts include upper-limit estimates. Accretion and chromospheric activity parameter counts include only non-negligible values. For the elemental abundances, the maximum number of derived values for each star/element is reported. See text for an explanation of the notation used.

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