Table B.1
Parameters needed to determine the temperature and gravity.
Star | V | K | π | σ(π) | E(B − V) | Mass∗ | T | g | [Fe/H] | ξ |
|
||||||||||
BD-01 2916 | 9.31 | 8.03 | 20.20 | 16.60 | 0.00 | – | 4480a | 1.20a | –1.99 | 2.4 |
BD+8 2856 | – | – | – | – | 0.00 | – | 4600a | 0.80a | –2.09 | 2.0 |
BD+30 2611 | 9.13 | 6.09 | 3.45 | 1.31 | 0.02 | – | 4238 | 0.50a | –1.20 | 1.7 |
BD+42 621 | 10.5 | 9.76 | 16.10 | 30.50 | 0.00 | – | 4725a | 1.50a | –2.48 | 1.7 |
BD+54 1323 | 9.34 | 7.37 | 1.22 | 1.20 | 0.01 | – | 5213 | 2.01c | –1.64 | 1.5 |
CS22890-024 | 13.41 | 11.44 | – | – | 0.05 | – | 5400 | 2.65a | –2.77 | 1.7 |
CS29512-073 | 13.92 | 12.51 | – | – | 0.05 | – | 5000a | 1.85a | –2.67 | 1.1 |
CS30312-100 | 13.05 | 10.88 | – | – | 0.08 | – | 5200 | 2.35a | –2.62 | 1.4 |
CS30312-059 | 13.14 | 10.70 | – | – | 0.12 | – | 5021 | 1.90a | –3.06 | 1.5 |
CS31082-001b | 11.67 | 9.46 | – | – | 0.00 | – | 4925 | 1.51a | –2.81 | 1.4 |
HD 74462 | 8.69 | 6.05 | 1.55 | 1.16 | 0.05 | – | 4590 | 1.84c | –1.48 | 1.1 |
HD 83212 | 8.33 | 5.61 | 1.96 | 0.98 | 0.05 | – | 4530 | 1.21c | –1.25 | 1.8 |
HD 88609b | 8.59 | 6.01 | 0.63 | 1.14 | 0.01 | – | 4568 | 1.01c | –2.87 | 1.9 |
HD 108317 | 8.03 | 6.15 | 4.53 | 1.06 | 0.01 | – | 5360 | 2.76 | –2.11 | 1.2 |
HD 110184 | 8.27 | 5.35 | 1.00 | 0.99 | 0.02 | – | 4450a | 0.50c | –2.40 | 2.1 |
HD 115444b | 8.96 | 6.61 | 3.55 | 1.12 | 0.01 | – | 4785 | 1.50c | –3.00 | 2.1 |
HD 122563b | 6.20 | 3.73 | 3.76 | – | 0.025 | – | 4560a | 0.90a | –2.81 | 1.8 |
HD 122956 | 7.25 | 5.90 | 3.30 | – | 0.083 | – | 4700 | 1.51 | –1.45 | 1.2 |
HD 126238 | 7.66 | 5.34 | 3.81 | 0.95 | 0.04 | – | 4900 | 1.80 | –1.92 | 1.5 |
HD 126587 | 9.11 | 6.668 | 1.40 | 1.44 | 0.09 | – | 4700a | 1.05c | –3.16 | 1.7 |
HD 128279 | 7.97 | 7.07 | 5.96 | – | 0.10 | – | 5200a | 2.20a | –2.34 | 1.3 |
HD 165195 | 7.34 | 4.14 | 2.20 | – | 0.195 | – | 4200c | 0.90c | –2.10 | 2.1 |
HD 166161b | 8.12 | 5.34 | 3.25 | 1.19 | 0.13 | – | 5250a | 2.15c | –1.25 | 1.9 |
HD 175305 | 7.18 | 5.06 | 6.18 | 0.56 | 0.03 | – | 5100 | 2.70 | –1.38 | 1.2 |
HD 186478 | 9.14 | 6.44 | 1.34 | 1.25 | 0.12 | – | 4730 | 1.50c | –2.42 | 1.8 |
HD 204543 | 8.28 | 5.78 | 1.08 | 1.38 | 0.04 | – | 4700 | 0.80a | –1.84 | 2.0 |
HE 0315+0000 | 15.52 | 13.20 | – | – | 0.081 | – | 5200 | 2.40a | –2.59 | 1.6 |
HE 0442-1234 | 12.91 | 9.96 | – | – | 0.133 | – | 4530 | 0.65a | –2.32 | 1.8 |
HE 1219-0312 | 15.94 | 13.89 | – | – | 0.00 | – | 4600 | 1.05a | –3.21 | 1.4 |
BD+092190 | 11.15 | 9.91 | 1.04 | 2.79 | 0.0281 | 0.8 | 6450a | 4.00 | –2.60 | 1.5 |
BD-133442 | 10.29 | 9.02 | – | – | 0.044 | 0.8 | 6450 | 4.20a | –2.56 | 1.5 |
CD-3018140 | 9.95 | 8.66 | 7.32 | 1.56 | 0.030 | 0.75 | 6340 | 4.13 | –1.92 | 1.0 |
CD-33 3337 | 9.08 | 7.67 | 9.11 | 1.01 | –0.0155 | 0.8 | 5952 | 3.95 | –1.55 | 1.4 |
CD-45 3283 | 10.57 | 8.97 | 15.32 | 1.38 | 0.0001 | 0.8 | 5657c | 4.97 | –0.99 | 0.8 |
CD-57 1633 | 9.53 | 8.09 | 10.68 | 0.91 | 0.0 | 0.8 | 5907 | 4.26 | –1.01 | 1.1 |
HD 3567 | 9.26 | 7.89 | 9.57 | 1.38 | –0.0028 | 0.82 | 6035 | 4.08 | –1.33 | 1.5 |
HD 19445 | 8.05 | 6.64 | 25.85 | 1.14 | –0.0014 | 0.70 | 5982 | 4.38 | –2.13 | 1.4 |
HD 22879 | 6.69 | 5.18 | 41.07 | 0.86 | –0.0056 | 0.8 | 5792 | 4.29 | –0.95 | 1.2 |
HD 25704 | 8.12 | 6.56 | 19.02 | 0.87 | –0.0211 | 0.8 | 5700 | 4.18 | –1.12 | 1.0 |
HD 63077 | 5.36 | 3.75 | 65.79 | 0.56 | –0.0225 | 0.8 | 5629 | 4.15 | –1.05 | 0.9 |
HD 63598 | 7.95 | 6.37 | 20.14 | 1.09 | 0.0 | 0.8 | 5680 | 4.16 | –0.99 | 0.9 |
HD 76932 | 5.80 | 4.36 | 46.90 | 0.97 | –0.024 | 0.85 | 5905 | 4.08 | –0.97 | 1.3 |
HD 103723 | 10.07 | 8.66 | 7.63 | 1.62 | 0.038 | 0.88 | 6128 | 4.28 | –0.85 | 1.5 |
HD 105004 | 10.31 | 8.87 | 2.68 | 4.49 | 0.038 | 0.8 | 5900a | 4.30c | –0.84 | 1.1 |
HD 106038b | 10.18 | 8.76 | 9.16 | 1.50 | –0.025 | 0.70 | 5950 | 4.33 | –1.48 | 1.1 |
HD 111980b | 8.37 | 6.77 | 12.48 | 1.38 | –0.0113 | 0.79 | 5653 | 3.90 | –1.31 | 1.2 |
HD 113679 | 9.70 | 8.11 | 6.82 | 1.32 | 0.024 | 0.96 | 5759 | 4.04 | –0.63 | 0.9 |
HD 116064 | 8.81 | 7.31 | 15.54 | 1.44 | 0.0352 | 0.8 | 5999 | 4.33 | –2.19 | 1.5 |
HD 120559 | 7.97 | 6.2 | 40.02 | 1.00 | 0.0070 | 0.8 | 5411 | 4.75 | –1.33 | 0.7 |
HD 121004 | 9.03 | 7.43 | 16.73 | 1.35 | 0.017 | 0.80 | 5711 | 4.46 | –0.73 | 0.7 |
HD 122196 | 8.73 | 7.28 | 9.77 | 1.32 | 0.032 | 0.78 | 6048 | 3.89 | –1.81 | 1.2 |
HD 126681b | 9.30 | 7.63 | 19.16 | 1.44 | –0.0183 | 0.70 | 5532 | 4.58 | –1.28 | 0.6 |
HD 132475 | 8.56 | 6.91 | 10.85 | 1.14 | 0.058 | 0.75 | 5838 | 3.90 | –1.52 | 1.5 |
HD 140283 | 7.21 | 5.59 | 17.44 | 0.97 | 0.021 | 0.75 | 5738 | 3.73 | –2.58 | 1.3 |
HD 160617 | 8.73 | 7.31 | 8.66 | 1.25 | 0.0155 | 0.82 | 6028 | 3.79 | –1.83 | 1.3 |
HD 166913 | 8.23 | 6.92 | 16.09 | 1.04 | –0.004 | 0.73 | 6155 | 4.07 | –1.30 | 1.5 |
HD 175179 | 9.07 | 7.54 | 11.85 | 1.52 | –0.0056 | 0.80 | 5758 | 4.16 | –0.72 | 0.9 |
HD 188510 | 8.83 | 7.13 | 25.32 | 1.17 | 0.0141 | 0.68 | 5536 | 4.63 | –1.58 | 1.0 |
HD 189558 | 7.74 | 6.16 | 14.76 | 1.10 | 0.0042 | 0.76 | 5712 | 3.79 | –1.18 | 1.2 |
HD 195633 | 8.55 | 7.10 | 8.63 | 1.16 | 0.0253 | 1.10 | 6005 | 3.86 | –0.71 | 1.4 |
HD 205650 | 9.05 | 7.57 | 18.61 | 1.23 | –0.007 | 0.70 | 5842 | 4.49 | –1.19 | 0.9 |
HD 213657 | 9.66 | 8.35 | 5.68 | 1.54 | 0.0099 | 0.77 | 6208 | 3.78 | –2.01 | 1.2 |
HD 298986 | 10.05 | 8.74 | 7.68 | 1.43 | 0.000 | 0.76 | 6144 | 4.18 | –1.48 | 1.4 |
G005-040 | 10.76 | 9.13 | – | – | 0.0366 | 0.8 | 5766 | 4.23a | –0.93 | 0.8 |
G013-009 | 10.0 | 8.74 | 5.75 | 1.55 | 0.027 | 0.76 | 6416 | 3.95 | –2.27 | 1.4 |
G020-024 | 11.13 | 9.67 | 5.42 | 2.32 | 0.118 | 0.78 | 6482 | 4.47 | –1.89 | 1.5 |
G064-012 | 11.46 | 10.21 | 1.88 | 2.90 | 0.042 | 0.8 | 6459 | 4.31c | –3.10 | 1.5 |
G064-037 | 11.14 | 9.92 | 2.88 | 3.10 | 0.0127 | 0.8 | 6494 | 3.82c | –3.17 | 1.4 |
G088-032 | 10.78 | 9.54 | 3.07 | 2.32 | –0.0028 | 0.80 | 6327 | 3.65 | –2.50 | 1.5 |
G088-040 | 8.93 | 7.51 | 12.15 | 1.24 | –0.0084 | 0.8 | 5929 | 4.14 | –0.90 | 1.4 |
G183-011 | 9.86 | 8.60 | 6.47 | 7.85 | 0.0084 | 0.70 | 6309 | 3.97 | –2.12 | 1.0 |
Notes. Top: Giants, bottom: Dwarfs. The superscripts a,b, and c indicate the following: (a) Stars with Teff and log g derived from excitation potential and ionisation balance. (b) Stars with a special r-process pattern – either r-poor or r-rich. (c) Stellar parameters were altered in accordance with (a) owing to uncertainties in colour, dereddening, and parallax.
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