Table B.1.
Stellar parameters and line abundances for each group spectrum.
| log g range | Teff [K] | [M/H] | n | S/N | Ba4554 | Fe4583 | Mg4702 | Ti4563 | Ti4571 |
|---|---|---|---|---|---|---|---|---|---|
| 2.005–2.007 | 4911 | −2.36 | 1 | 120 | 0.01 − 0.55 | 5.03 − 5.33 | 5.37 − 5.60 | 2.60 − 3.13 | 2.83 − 3.40 |
| 2.007–2.083 | 4912 | −2.42 | 1 | 104 | 0.04 − 0.57 | 5.04 − 5.33 | 5.20 − 5.41 | 2.63 − 3.17 | 2.96 − 3.53 |
| 2.083–2.126 | 4949 | −2.49 | 2 | 148 | 0.02 − 0.56 | 5.04 − 5.34 | 5.36 − 5.58 | 2.59 − 3.11 | 2.96 − 3.52 |
| 2.126–2.22 | 4975 | −2.41 | 2 | 154 | 0.00 − 0.55 | 5.01 − 5.31 | 5.25 − 5.45 | 2.59 − 3.10 | 2.87 − 3.44 |
| 2.22–2.283 | 4997 | −2.45 | 2 | 138 | 0.00 − 0.55 | 5.03 − 5.32 | 5.32 − 5.53 | 2.52 − 3.04 | 2.83 − 3.39 |
| 2.283–2.331 | 5019 | −2.44 | 2 | 134 | 0.04 − 0.58 | 4.99 − 5.28 | 5.37 − 5.58 | 2.60 − 3.11 | 2.79 − 3.35 |
| 2.331–2.414 | 5047 | −2.44 | 2 | 119 | −0.00 to 0.55 | 5.02 − 5.30 | 5.42 − 5.62 | 2.56 − 3.07 | 2.93 − 3.50 |
| 2.414–2.467 | 5072 | −2.34 | 3 | 129 | 0.20 − 0.68 | 5.11 − 5.41 | 5.44 − 5.65 | 2.65 − 3.16 | 2.94 − 3.50 |
| 2.467–2.661 | 5112 | −2.37 | 3 | 124 | 0.18 − 0.67 | 5.06 − 5.35 | 5.29 − 5.47 | 2.71 − 3.22 | 2.91 − 3.45 |
| 2.661–2.676 | 5151 | −2.43 | 3 | 106 | 0.10 − 0.63 | 5.08 − 5.37 | 5.31 − 5.48 | 2.61 − 3.09 | 2.96 − 3.50 |
| 2.676–2.768 | 5166 | −2.40 | 4 | 117 | 0.09 − 0.61 | 5.01 − 5.28 | 5.36 − 5.54 | 2.64 − 3.14 | 2.94 − 3.49 |
| 2.768–2.842 | 5193 | −2.35 | 5 | 110 | −0.07 to 0.50 | 5.01 − 5.27 | 5.34 − 5.51 | 2.52 − 2.97 | 2.75 − 3.25 |
| 2.842–2.909 | 5220 | −2.31 | 3 | 117 | 0.09 − 0.61 | 5.06 − 5.32 | 5.31 − 5.46 | 2.59 − 3.03 | 2.89 − 3.40 |
| 2.909–2.96 | 5232 | −2.36 | 2 | 114 | 0.11 − 0.62 | 5.10 − 5.37 | 5.37 − 5.53 | 2.67 − 3.14 | 2.83 − 3.34 |
| 2.96–3.153 | 5268 | −2.37 | 8 | 107 | 0.10 − 0.61 | 5.05 − 5.30 | 5.27 − 5.41 | 2.67 − 3.11 | 2.88 − 3.38 |
| 3.153–3.275 | 5338 | −2.41 | 6 | 94 | 0.06 − 0.58 | 5.19 − 5.46 | 5.27 − 5.40 | 2.65 − 3.06 | 2.90 − 3.38 |
| 3.275–3.341 | 5377 | −2.42 | 5 | 106 | −0.09 to 0.48 | 5.07 − 5.31 | 5.28 − 5.41 | 2.76 − 3.20 | 2.88 − 3.35 |
| 3.341–3.459 | 5423 | −2.44 | 9 | 94 | −0.23 to 0.36 | 4.99 − 5.21 | 5.40 − 5.53 | 2.65 − 3.05 | 2.72 − 3.14 |
| 3.459–3.532 | 5544 | −2.44 | 4 | 83 | −0.41 to 0.17 | 5.03 − 5.27 | 5.27 − 5.39 | 2.68 − 3.06 | 2.74 − 3.17 |
| 3.532–3.589 | 5643 | −2.42 | 4 | 83 | −0.33 to 0.27 | 5.06 − 5.31 | 5.38 − 5.49 | 2.58 − 2.89 | 2.72 − 3.12 |
| 3.589–3.61 | 5704 | −2.45 | 4 | 87 | −0.32 to 0.32 | 5.01 − 5.24 | 5.32 − 5.43 | 2.60 − 2.90 | 2.65 − 3.01 |
| 3.61–3.666 | 5746 | −2.43 | 6 | 88 | −0.56 to −0.04 | 5.03 − 5.28 | 5.36 − 5.48 | 2.67 − 2.99 | 2.64 − 2.96 |
| 3.666–3.726 | 5878 | −2.42 | 5 | 86 | −0.50 to −0.01 | 4.89 − 5.08 | 5.35 − 5.48 | 2.42 − 2.62 | 2.72 − 3.07 |
| 3.726–3.802 | 6000 | −2.40 | 5 | 86 | −0.68 to −0.37 | 5.07 − 5.29 | 5.30 − 5.42 | 2.63 − 2.88 | 2.68 − 2.97 |
| 3.802–3.832 | 6099 | −2.42 | 4 | 78 | −0.59 to −0.23 | 4.97 − 5.17 | 5.22 − 5.34 | 2.58 − 2.79 | 2.72 − 3.00 |
| 3.832–3.883 | 6164 | −2.39 | 8 | 91 | −0.68 to −0.30 | 5.01 − 5.22 | 5.24 − 5.38 | 2.65 − 2.88 | 2.65 − 2.89 |
| 3.883–3.917 | 6237 | −2.51 | 8 | 85 | −0.69 to −0.39 | 4.93 − 5.11 | 5.23 − 5.38 | 2.67 − 2.86 | 2.73 − 2.99 |
| 3.917–3.95 | 6276 | −2.48 | 8 | 84 | −0.78 to −0.37 | 5.00 − 5.21 | 5.24 − 5.39 | 2.61 − 2.79 | 2.71 − 2.98 |
| 3.95–3.972 | 6320 | −2.50 | 6 | 77 | −0.82 to −0.24 | 4.90 − 5.08 | 5.27 − 5.42 | 2.63 − 2.80 | 2.69 − 2.93 |
| 3.972–4.003 | 6351 | −2.48 | 8 | 82 | −0.83 to −0.60 | 4.90 − 5.07 | 5.28 − 5.45 | 2.70 − 2.91 | 2.77 − 3.02 |
| 4.003–4.025 | 6377 | −2.50 | 7 | 79 | −0.64 to −0.21 | 5.04 − 5.24 | 5.26 − 5.40 | 2.63 − 2.81 | 2.72 − 2.94 |
| 4.025–4.038 | 6390 | −2.49 | 6 | 72 | −0.57 to −0.33 | 4.97 − 5.18 | 5.35 − 5.47 | 2.61 − 2.79 | 2.82 − 3.06 |
| 4.038–4.066 | 6403 | −2.50 | 7 | 71 | −0.70 to 0.41 | 5.01 − 5.24 | 5.32 − 5.45 | 2.65 − 2.82 | 2.73 − 2.96 |
| 4.066–4.21 | 6429 | −2.50 | 8 | 72 | −0.94 to −0.70 | 4.99 − 5.16 | 5.26 − 5.48 | 2.81 − 3.04 | 2.93 − 3.20 |
Notes. For each line the smallest and greatest abundance found when varying the continuum level and assumed vmic is shown. Statistical errors are generally in the range 0.03 − 0.05, much smaller than the systematic errors. This includes abundances that are never actually used in the model fitting, such as for the Ba4554 line.
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