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Table A.3

Carbon abundance obtained from the CH G band, for stars observed with MIKE (except for star #12, see text) and UVES.

Star # [C/H] [C/Fe] Star # [C/H] [C/Fe]

08 6.92 ± 0.04 −0.43 19 5.01 ± 0.01 −0.56
09 5.79 ± 0.01 −0.50 20 4.48 ± 0.02 −0.95
10 6.52 ± 0.03 −0.31 21 7.21 ± 0.02 −0.57
11 6.97 ± 0.04 −0.62 22 6.77 ± 0.02 −0.46
13 6.69 ± 0.05 −0.72 23 6.12 ± 0.01 −0.49
14 6.80 ± 0.03 −0.42 24 5.30 ± 0.01 −0.52
15 6.72 ± 0.02 −0.50 25 6.64 ± 0.03 −0.64
16 6.57 ± 0.04 −0.68 26 6.27 ± 0.01 −0.53
17 6.79 ± 0.02 −0.44 27 7.75 ± 0.03 −0.18
18 6.68 ± 0.03 −0.65 28 6.41 ± 0.02 −0.89

Notes. The error given is the formal one provided by the fit and should be considered as an indication of its quality. A more realistic error would amount to ~0.2 dex, taking into account the uncertainties on the continuum, oxygen abundance, and stellar parameters (especially Teff). The adopted C-solar abundance is 8.55 as in Jablonka et al. (2015).

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