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Table 3

Parameters and abundances of the program stars.

Star Teff (K) log g (dex) [Fe/H] (dex) υmic (km s−1) υmac (km s−1) [C/Fe] (dex) [N/Fe] (dex) [O/Fe] (dex) [F/Fe] (dex) [F/H] (dex) [Ce/Fe] (dex) [Ce/H] (dex)
N7789_1 3811 1.20 0.00 1.76 6.30 −0.18 0.26 −0.04 −0.13±0.11 −0.13±0.15 0.09±0.11 0.09±0.15
N7789_2 3802 1.20 0.02 1.68 5.96 −0.18 0.21 −0.05 −0.10±0.11 −0.09±0.15 0.05±0.07 0.07±0.12
N7789_4 3930 1.43 0.00 1.55 6.28 −0.18 0.25 −0.04 −0.12±0.14 −0.13±0.17 0.13±0.09 0.13±0.16

N7044_1 3817 1.30 0.11 1.75 6.78 −0.19 0.26 −0.08 −0.12±0.08 −0.02±0.13 0.04±0.08 0.15±0.13
N7044_2 3852 1.32 0.06 1.72 6.93 −0.17 0.27 −0.06 −0.09±0.11 −0.03±0.15 0.00±0.07 0.06±0.12
N7044_3 3890 1.39 0.06 1.66 7.02 −0.20 0.26 −0.06 −0.12±0.13 −0.05±0.16 0.02±0.10 0.08±0.14
N7044_4 3877 1.39 0.08 1.67 6.61 −0.19 0.24 −0.07 −0.16±0.13 −0.08±0.16 0.03±0.07 0.11±0.12

N6819_a 3542 0.71 −0.02 1.83 5.85 −0.14 0.15 −0.03 0.00±0.10 −0.03±0.14 −0.20±0.08 −0.22±0.13
N6819_b 3590 0.79 −0.02 1.82 6.16 −0.14 0.11 −0.03 −0.01±0.08 −0.03±0.13 −0.15±0.08 −0.17±0.13

Rup171_1 3881 1.36 0.02 1.60 6.77 −0.16 0.23 −0.05 −0.08±0.12 −0.06±0.16 −0.04±0.10 −0.02±0.14
Rup171_2 4012 1.62 0.03 1.51 6.72 −0.17 0.19 −0.06 −0.12±0.12 −0.08±0.16 0.01±0.08 0.03±0.13

Trumpler5_1 3582 0.58 −0.40 1.99 6.98 −0.11 0.19 0.10 0.01±0.09 −0.39±0.13 0.09±0.08 −0.31±0.13

King11_1 3356 0.28 −0.25 1.90 10.25 −0.17 0.21 0.05 −0.04±0.07 −0.29±0.12 −0.18±0.09 −0.43±0.13
King11_2 3711 0.86 −0.25 1.85 6.39 −0.11 0.13 0.05 −0.11±0.10 −0.36±0.14 −0.01±0.07 −0.26±0.12
King11_3 4083 1.56 −0.24 1.57 6.78 −0.13 0.21 0.05 −0.02±0.14 −0.26±0.17 0.11±0.08 −0.13±0.13

N6791_2 3493 0.83 0.25 1.81 6.50 0.05 0.10 0.06 0.26±0.10 0.51±0.14 −0.24±0.08 0.01±0.13
N6791_3 3490 0.87 0.27 1.76 6.39 0.02 0.14 0.06 0.34±0.11 0.61±0.15 −0.21±0.08 0.06±0.13

Notes. Abundance ratios are scaled to the solar values of A(C) = 8.46, A(N) = 7.83, A(O) = 8.69, A(F) = 4.40, A(Fe) = 7.46, and A(Ce) = 1.58 (Asplund et al. 2021). Typical uncertainties of the derived stellar parameters are ±100 K in Teff, ±0.2 dex in log g, ±0.1 dex in [Fe/H], ±0.1 km s−1 in υmic, ±0.1 dex in [C/Fe], and ±0.1 dex in [N/Fe].

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