Table C.2.
Elemental abundances of sample stars, along with the standard deviation due to line-to-line scatter.
| Z | log ϵ⊙ | log ϵ | N | [X/H] | [X/Fe] | σ[X/Fe] | log ϵ | N | [X/H] | [X/Fe] | σ[X/Fe] | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| HR Peg | HD 288833 | |||||||||||
| C | 6 | 8.43 | 8.05 | – | −0.37 | −0.02 | 0.17 | 8.05 | – | −0.37 | −0.06 | 0.17 |
| N | 7 | 7.83 | 8.45 ± 0.10 | – | 0.62 | 0.97 | 0.64 | 8.60 ± 0.13 | – | 0.77 | 1.07 | 0.64 |
| O | 8 | 8.69 | 8.36 | – | −0.33 | 0.02 | – | 8.36 | – | −0.33 | −0.02 | – |
| Fe | 26 | 7.50 | 7.15 ± 0.18 | 14 | −0.35 | – | 0.22 | 7.19 ± 0.14 | 13 | −0.30 | – | 0.19 |
| Y I | 39 | 2.21 | 2.30 ± 0.00 | 1 | 0.09 | 0.44 | 0.25 | 2.50 ± 0.00 | 1 | 0.29 | 0.59 | 0.19 |
| Y II | 39 | 2.21 | 1.90 ± 0.00 | 1 | −0.31 | 0.04 | 0.25 | – | – | – | – | – |
| Zr I | 40 | 2.58 | 2.85 ± 0.21 | 2 | 0.27 | 0.62 | 0.23 | 2.75 ± 0.07 | 2 | 0.17 | 0.47 | 0.12 |
| Nb I | 41 | 1.46 | 1.35 ± 0.21 | 2 | −0.11 | 0.24 | 0.23 | 1.30 ± 0.17 | 3 | −0.16 | 0.14 | 0.19 |
| Tc I | 43 | – | −1.30 ± 0.00 | 1 | – | – | – | −1.20 ± 0.00 | 1 | – | – | – |
| Ba I | 56 | 2.18 | 1.90 ± 0.00 | 1 | −0.28 | 0.07 | 0.17 | – | – | – | – | |
| Ce II | 58 | 1.58 | 1.22 ± 0.25 | 5 | −0.36 | −0.01: | 0.17 | 1.38 ± 0.29 | 6 | −0.20 | 0.10 | 0.33 |
| Pr II | 59 | 0.72 | 1.00 ± 0.00 | 1 | 0.28 | 0.63 | 0.14 | 1.05 ± 0.21 | 2 | 0.33 | 0.63 | 0.22 |
| Nd II | 60 | 1.42 | 1.53 ± 0.05 | 3 | 0.11 | 0.46 | 0.22 | 1.42 ± 0.15 | 4 | 0.01 | 0.31 | 0.26 |
| Eu II | 63 | 0.52 | 0.20 ± 0.00 | 2 | −0.32 | 0.03 | 0.14 | 0.60 ± 0.14 | 2 | 0.08 | 0.38 | 0.17 |
| AA Cam | V1139 Tau | |||||||||||
| C | 6 | 8.43 | 8.06 | – | −0.37 | −0.04 | 0.25 | 8.53 | – | 0.11 | 0.17 | 0.17 |
| N | 7 | 7.83 | 8.40 ± 0.13 | – | 0.57 | 0.89 | 0.65 | 9.90 ± 0.15 | – | 2.07 | 2.13 | 0.65 |
| O | 8 | 8.69 | 8.36 | – | −0.33 | 0.00 | – | 8.66 | −0.03 | 0.03 | ||
| Fe | 26 | 7.50 | 7.17 ± 0.12 | 15 | −0.33 | – | 0.18 | 7.44 ± 0.13 | 14 | −0.06 | – | 0.19 |
| Y I | 39 | 2.21 | 1.90 ± 0.00 | 1 | −0.31 | 0.02 | 0.22 | – | – | – | – | – |
| Y II | 39 | 2.21 | 2.20 ± 0.00 | 1 | −0.01 | 0.32 | 0.22 | – | – | – | – | – |
| Zr I | 40 | 2.58 | 2.75 ± 0.21 | 2 | 0.17 | 0.49 | 0.23 | 2.80 ± 0.00 | 1 | 0.22 | 0.28 | 0.14 |
| Nb I | 41 | 1.46 | 1.30 ± 0.17 | 3 | −0.16 | 0.16 | 0.19 | 1.35 ± 0.21 | 2 | −0.11 | −0.05 | 0.23 |
| Tc I | 43 | – | −0.40 ± 0.00 | 1 | – | – | – | −0.60 ± 0.00 | 1 | – | – | – |
| Ba I | 56 | 2.18 | 1.90 ± 0.0 | 1 | −0.28 | 0.05 | 0.17 | 2.40 ± 0.00 | 1 | 0.22 | 0.28 | 0.17 |
| Ce II | 58 | 1.58 | 1.24 ± 0.28 | 6 | −0.34 | −0.01: | 0.15 | 1.90 ± 0.10 | 3 | 0.32 | 0.38 | 0.17 |
| Nd II | 60 | 1.42 | 1.30 ± 0.17 | 3 | −0.12 | 0.21 | 0.17 | – | – | – | – | – |
| KR CMa | CSS 151 | |||||||||||
| C | 6 | 8.43 | 8.36 | – | −0.07 | −0.06 | 0.17 | 8.06 | – | −0.37 | −0.11 | 0.26 |
| N | 7 | 7.83 | 8.80 ± 0.18 | – | 0.97 | 0.98 | 0.66 | 8.60 ± 0.12 | – | 0.77 | 1.03 | 0.65 |
| O | 8 | 8.69 | 8.66 | – | −0.03 | −0.01 | – | 8.36 | – | −0.33 | −0.07 | |
| Fe | 26 | 7.50 | 7.48 ± 0.18 | 14 | −0.01 | – | 0.22 | 7.24 ± 0.14 | 14 | −0.26 | 0 | 0.19 |
| Y I | 39 | 2.21 | 2.80 ± 0.00 | 1 | 0.59 | 0.60 | 0.14 | 2.50 ± 0.00 | 1 | 0.29 | 0.54 | 0.31 |
| Zr I | 40 | 2.58 | – | – | – | – | – | 2.95 ± 0.21 | 2 | 0.37 | 0.63 | 0.23 |
| Tc I | 43 | – | – | – | – | – | – | −0.10 ± 0.00 | 1 | – | – | – |
| Ba I | 56 | 2.18 | 2.50 ± 0.00 | 1 | 0.32 | 0.33 | 0.17 | 2.20 ± 0.00 | 1 | 0.02 | 0.28 | 0.17 |
| Ce II | 58 | 1.58 | 1.70 ± 0.30 | 4 | 0.12 | 0.13 | 0.22 | 1.81 ± 0.28 | 6 | 0.23 | 0.48 | 0.17 |
| Pr II | 59 | 0.72 | – | – | – | – | – | 0.90 ± 0.00 | 1 | 0.18 | 0.43 | 0.14 |
| Nd II | 60 | 1.42 | 2.30 ± 0.00 | 1 | 0.88 | 0.89 | 0.24 | 1.57 ± 0.30 | 4 | 0.15 | 0.41 | 0.37 |
| Sm II | 62 | 0.96 | – | – | – | – | – | 1.10 ± 0.00 | 1 | 0.14 | 0.40 | 0.14 |
| Eu II | 63 | 0.52 | – | – | – | – | – | 0.50 ± 0.00 | 1 | −0.02 | 0.24 | 0.14 |
Notes. Solar abundances (third column) are from Asplund et al. (2009). The column labelled N lists the number of lines used to derive the corresponding abundance. The σ[X/Fe] column lists the total uncertainty on the abundance calculated using the method described in Sect. 5.8. Colons flag uncertain values.
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