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Table A.1
LTE and non-LTE copper abundance ratios [Cu/Fe] for stars with VLT/UVES spectra.
| Star | Teff (K) | log g | [Fe/H] | ξ | [α/Fe] | 5105 Å | 5218 Å | 5782 Å | [Cu/Fe] | Class | LFS |
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| BD−21 3420 | 5808 | 4.26 | −1.13 | 1.30 | 0.31 | −0.39 | −0.35 | ... | −0.37 ± 0.03 | TD | L |
| − | − | − | − | − | −0.28 | −0.30 | ... | −0.29 ± 0.01 | N | ||
| CD−33 3337 | 5979 | 3.86 | −1.36 | 1.70 | 0.30 | −0.32 | −0.21 | ... | −0.26 ± 0.08 | TD | L |
| − | − | − | − | − | −0.09 | −0.04 | ... | −0.06 ± 0.04 | N | ||
| CD−43 6810 | 5945 | 4.26 | −0.43 | 1.30 | 0.23 | −0.07 | −0.06 | ... | −0.07 ± 0.01 | high-α | L |
| − | − | − | − | − | −0.01 | −0.03 | ... | −0.02 ± 0.01 | N | ||
| CD−45 3283 | 5597 | 4.55 | −0.91 | 1.00 | 0.12 | −0.59 | −0.56 | ... | −0.57 ± 0.02 | low-α | L |
| − | − | − | − | − | −0.54 | −0.55 | ... | −0.54 ± 0.01 | N | ||
| CD−57 1633 | 5873 | 4.28 | −0.90 | 1.20 | 0.07 | −0.74 | −0.66 | ... | −0.70 ± 0.06 | low-α | L |
| − | − | − | − | − | −0.66 | −0.62 | ... | −0.64 ± 0.03 | N | ||
| CD−61 282 | 5759 | 4.31 | −1.23 | 1.30 | 0.22 | −0.73 | −0.66 | ... | −0.69 ± 0.05 | low-α | L |
| − | − | − | − | − | −0.63 | −0.62 | ... | −0.63 ± 0.01 | N | ||
| G05-19 | 5854 | 4.26 | −1.18 | 1.30 | 0.19 | −0.70 | ... | ... | −0.70 ± 0.00 | low-α | L |
| − | − | − | − | − | −0.58 | ... | ... | −0.58 ± 0.00 | N | ||
| G05-40 | 5795 | 4.17 | −0.81 | 1.20 | 0.31 | −0.22 | −0.20 | ... | −0.21 ± 0.01 | high-α | L |
| − | − | − | − | − | −0.14 | −0.16 | ... | −0.15 ± 0.01 | N | ||
| G18-28 | 5372 | 4.41 | −0.83 | 1.00 | 0.31 | −0.11 | −0.14 | ... | −0.13 ± 0.02 | high-α | L |
| − | − | − | − | − | −0.06 | −0.03 | ... | −0.05 ± 0.02 | N | ||
| G18-39 | 6040 | 4.21 | −1.39 | 1.50 | 0.34 | −0.59 | ... | ... | −0.59 ± 0.00 | high-α | L |
| − | − | − | − | − | −0.39 | ... | ... | −0.39 ± 0.00 | N | ||
| G46-31 | 5901 | 4.23 | −0.83 | 1.40 | 0.15 | −0.42 | −0.31 | ... | −0.37 ± 0.08 | low-α | L |
| − | − | − | − | − | −0.33 | −0.26 | ... | −0.30 ± 0.05 | N | ||
| G66-22 | 5236 | 4.41 | −0.86 | 0.90 | 0.12 | −0.51 | −0.54 | ... | −0.52 ± 0.02 | low-α | L |
| − | − | − | − | − | −0.48 | −0.54 | ... | −0.51 ± 0.04 | N | ||
| G82-05 | 5277 | 4.45 | −0.75 | 0.90 | 0.09 | −0.59 | −0.57 | ... | −0.58 ± 0.01 | low-α | L |
| − | − | − | − | − | −0.56 | −0.57 | ... | −0.56 ± 0.01 | N | ||
| G112-43 | 6074 | 4.03 | −1.25 | 1.30 | 0.24 | −0.58 | −0.53 | ... | −0.55 ± 0.04 | low-α | L |
| − | − | − | − | − | −0.39 | −0.39 | ... | −0.39 ± 0.00 | N | ||
| G112-44 | 5819 | 4.25 | −1.29 | 1.20 | 0.22 | −0.54 | −0.48 | ... | −0.51 ± 0.04 | low-α | L |
| − | − | − | − | − | −0.41 | −0.41 | ... | −0.41 ± 0.00 | N | ||
| G114-42 | 5643 | 4.38 | −1.10 | 1.30 | 0.19 | −0.43 | −0.36 | ... | −0.40 ± 0.05 | low-α | L |
| − | − | − | − | − | −0.35 | −0.33 | ... | −0.34 ± 0.01 | N | ||
| G121-12 | 5928 | 4.23 | −0.93 | 1.40 | 0.10 | −0.73 | ... | ... | −0.73 ± 0.00 | low-α | L |
| − | − | − | − | − | −0.63 | ... | ... | −0.63 ± 0.00 | N | ||
| G159-50 | 5624 | 4.37 | −0.93 | 1.10 | 0.31 | −0.24 | −0.21 | ... | −0.22 ± 0.02 | high-α | L |
| − | − | − | − | − | −0.17 | −0.19 | ... | −0.18 ± 0.01 | N | ||
| G188-22 | 5974 | 4.18 | −1.32 | 1.50 | 0.35 | −0.41 | ... | ... | −0.41 ± 0.00 | high-α | L |
| − | − | − | − | − | −0.24 | ... | ... | −0.24 ± 0.00 | N | ||
| HD 3567 | 6051 | 4.02 | −1.16 | 1.50 | 0.21 | −0.73 | ... | ... | −0.73 ± 0.00 | low-α | L |
| − | − | − | − | − | −0.55 | ... | ... | −0.55 ± 0.00 | N | ||
| HD 17820 | 5773 | 4.22 | −0.67 | 1.30 | 0.29 | −0.10 | −0.10 | ... | −0.10 ± 0.00 | TD | L |
| − | − | − | − | − | −0.03 | −0.07 | ... | −0.05 ± 0.03 | N | ||
| HD 22879 | 5759 | 4.25 | −0.85 | 1.30 | 0.31 | −0.22 | −0.18 | ... | −0.20 ± 0.03 | TD | L |
| − | − | − | − | − | −0.14 | −0.14 | ... | −0.14 ± 0.00 | N | ||
| HD 25704 | 5868 | 4.26 | −0.85 | 1.40 | 0.24 | −0.16 | −0.18 | ... | −0.17 ± 0.01 | TD | L |
| − | − | − | − | − | −0.07 | −0.13 | ... | −0.10 ± 0.04 | N | ||
| HD 51754 | 5767 | 4.29 | −0.58 | 1.40 | 0.26 | −0.05 | −0.09 | ... | −0.07 ± 0.03 | high-α | L |
| − | − | − | − | − | 0.01 | −0.06 | ... | −0.03 ± 0.05 | N | ||
| HD 76932 | 5877 | 4.13 | −0.87 | 1.40 | 0.29 | −0.19 | −0.18 | ... | −0.18 ± 0.01 | TD | L |
| − | − | − | − | − | −0.09 | −0.12 | ... | −0.11 ± 0.02 | N | ||
| HD 97320 | 6008 | 4.19 | −1.17 | 1.60 | 0.28 | −0.28 | −0.21 | ... | −0.24 ± 0.05 | TD | L |
| − | − | − | − | − | −0.13 | −0.11 | ... | −0.12 ± 0.01 | N | ||
| HD 103723 | 5938 | 4.19 | −0.80 | 1.20 | 0.14 | −0.53 | −0.50 | ... | −0.51 ± 0.02 | low-α | L |
| − | − | − | − | − | −0.44 | −0.45 | ... | −0.45 ± 0.01 | N | ||
| HD 105004 | 5754 | 4.30 | −0.82 | 1.20 | 0.14 | −0.28 | −0.25 | ... | −0.27 ± 0.02 | low-α | L |
| − | − | − | − | − | −0.21 | −0.22 | ... | −0.22 ± 0.01 | N | ||
| HD 106516 | 6196 | 4.42 | −0.68 | 1.30 | 0.29 | −0.14 | −0.12 | ... | −0.13 ± 0.01 | TD | L |
| − | − | − | − | − | −0.06 | −0.07 | ... | −0.06 ± 0.01 | N | ||
| HD 111980 | 5778 | 3.96 | −1.08 | 1.50 | 0.34 | −0.38 | −0.34 | ... | −0.36 ± 0.03 | high-α | L |
| − | − | − | − | − | −0.25 | −0.27 | ... | −0.26 ± 0.01 | N | ||
| HD 113679 | 5672 | 3.99 | −0.65 | 1.40 | 0.32 | −0.13 | −0.13 | ... | −0.13 ± 0.00 | high-α | L |
| − | − | − | − | − | −0.06 | −0.10 | ... | −0.08 ± 0.03 | N | ||
| HD 114762A | 5856 | 4.21 | −0.70 | 1.50 | 0.24 | −0.12 | −0.11 | ... | −0.11 ± 0.01 | TD | L |
| − | − | − | − | − | −0.04 | −0.07 | ... | −0.06 ± 0.02 | N | ||
| HD 120559 | 5412 | 4.50 | −0.89 | 1.10 | 0.30 | −0.06 | −0.10 | ... | −0.08 ± 0.03 | TD | L |
| − | − | − | − | − | −0.01 | −0.09 | ... | −0.05 ± 0.06 | N | ||
| HD 121004 | 5669 | 4.37 | −0.70 | 1.30 | 0.32 | −0.12 | −0.15 | ... | −0.13 ± 0.02 | high-α | L |
| − | − | − | − | − | −0.06 | −0.13 | ... | −0.09 ± 0.05 | N | ||
| HD 126681 | 5507 | 4.45 | −1.17 | 1.20 | 0.35 | −0.33 | −0.28 | ... | −0.31 ± 0.04 | TD | L |
| − | − | − | − | − | −0.26 | −0.26 | ... | −0.26 ± 0.00 | N | ||
| HD 132475 | 5646 | 3.76 | −1.49 | 1.50 | 0.38 | −0.49 | −0.37 | ... | −0.43 ± 0.08 | ? high-α | L |
| − | − | − | − | − | −0.30 | −0.26 | ... | −0.28 ± 0.03 | N | ||
| HD 148816 | 5823 | 4.13 | −0.73 | 1.40 | 0.27 | −0.10 | −0.11 | ... | −0.10 ± 0.01 | high-α | L |
| − | − | − | − | − | −0.02 | −0.07 | ... | −0.05 ± 0.04 | N | ||
| HD 163810 | 5501 | 4.56 | −1.20 | 1.30 | 0.21 | −0.52 | −0.56 | ... | −0.54 ± 0.03 | low-α | L |
| − | − | − | − | − | −0.46 | −0.55 | ... | −0.50 ± 0.06 | N | ||
| HD 175179 | 5713 | 4.33 | −0.65 | 1.20 | 0.29 | −0.09 | −0.12 | ... | −0.11 ± 0.02 | TD | L |
| − | − | − | − | − | −0.03 | −0.10 | ... | −0.06 ± 0.05 | N | ||
| HD 179626 | 5850 | 4.13 | −1.04 | 1.60 | 0.31 | −0.35 | −0.27 | ... | −0.31 ± 0.06 | high-α | L |
| − | − | − | − | − | −0.23 | −0.20 | ... | −0.21 ± 0.02 | N | ||
| HD 189558 | 5617 | 3.80 | −1.12 | 1.40 | 0.33 | −0.43 | −0.36 | ... | −0.40 ± 0.05 | TD | L |
| − | − | − | − | − | −0.31 | −0.30 | ... | −0.31 ± 0.01 | N | ||
| HD 193901 | 5656 | 4.36 | −1.09 | 1.20 | 0.16 | −0.67 | −0.56 | ... | −0.62 ± 0.08 | low-α | L |
| − | − | − | − | − | −0.59 | −0.53 | ... | −0.56 ± 0.04 | N | ||
| HD 194598 | 5942 | 4.33 | −1.09 | 1.40 | 0.18 | −0.46 | −0.44 | ... | −0.45 ± 0.01 | low-α | L |
| − | − | − | − | − | −0.35 | −0.38 | ... | −0.37 ± 0.02 | N | ||
| HD 199289 | 5810 | 4.28 | −1.04 | 1.30 | 0.30 | −0.20 | −0.15 | ... | −0.17 ± 0.04 | TD | L |
| − | − | − | − | − | −0.10 | −0.10 | ... | −0.10 ± 0.00 | N | ||
| HD 205650 | 5698 | 4.32 | −1.17 | 1.30 | 0.30 | −0.25 | −0.18 | ... | −0.21 ± 0.05 | TD | L |
| − | − | − | − | − | −0.15 | −0.14 | ... | −0.14 ± 0.01 | N | ||
| HD 222766 | 5334 | 4.27 | −0.67 | 0.80 | 0.30 | −0.12 | −0.15 | ... | −0.13 ± 0.02 | high-α | L |
| − | − | − | − | − | −0.08 | −0.14 | ... | −0.11 ± 0.04 | N | ||
| HD 241253 | 5831 | 4.31 | −1.10 | 1.30 | 0.29 | −0.28 | −0.23 | ... | −0.25 ± 0.04 | TD | L |
| − | − | − | − | − | −0.17 | −0.18 | ... | −0.17 ± 0.01 | N | ||
Notes. The stellar parameters including [α/Fe] are the same as Nissen & Schuster (2010). Columns 7–9 are the abundance ratios derived from corresponding Cu i lines, and Col. 10 presents both stellar LTE and non-LTE copper abundance ratios (for each star, first and second row, respectively), and the line-to-line scatter is also provided in this column (following the “±” sign). The classification is indicated by “TD” (thick-disk), “high-α” and “low-α”, and a “?” are added if the classification is uncertain. The rightmost column shows the line formation scenario for each star, where “L” represents LTE line formation and “N” represents non-LTE line formation. The stars without available copper abundance are not listed in the table.
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