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 |
Ṁ 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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