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Table 1.
Astrophysical parameters and their errors, taken from Kinman et al. (2000) and Behr (2003) according to the column “Ref”.
| Star | TYC | V | Teff | log g | [M/H] | [Fe/H] | υ sin i | Ref |
|---|---|---|---|---|---|---|---|---|
| (mag) | (K) | (dex) | (dex) | (km s−1) | ||||
| BD−07 230 | 4684-1840-1 | 11.13 | 9647 ± 269 | 3.40 ± 0.33 | −0.44 ± 0.11 | 2 | 2 | |
| BD+01 548 | 55-357-1 | 10.76 | 8714 ± 198 | 3.38 ± 0.16 | −2.23 ± 0.06 | 10 | 2 | |
| BD+25 2602 | 1994-1778-1 | 10.10 | 8410 ± 100 | 3.17 ± 0.04 | –2.0 | −2.08 ± 0.11 | 12 | 1 |
| BD+42 2309 | 3020-678-1 | 10.84 | 8825 ± 88 | 3.20 ± 0.05 | –1.5 | −1.69 ± 0.05 | 35 | 1 |
| HD 2857 | 4678-90-1 | 9.90 | 7566 ± 58 | 3.00 ± 0.08 | –1.5 | −1.67 ± 0.11 | 30 | 1 |
| HD 4580 | 3659-586-1 | 8.78 | 8453 ± 80 | 3.20 ± 0.08 | –1.5 | 14 | 1 | |
| HD 8376 | 2292-1267-1 | 9.60 | 8133 ± 48 | 3.27 ± 0.04 | –2.5 | 10 | 1 | |
| HD 13780 | 8045-420-1 | 9.82 | 7930 ± 23 | 3.12 ± 0.02 | –1.5 | 14 | 1 | |
| HD 14829 | 5282-1684-1 | 10.30 | 9086 ± 245 | 3.31 ± 0.19 | −2.01 ± 0.31 | 14 | 2 | |
| HD 31943 | 7593-771-1 | 8.26 | 7893 ± 59 | 3.22 ± 0.11 | –1.0 | 7 | 1 | |
| HD 60778 | 4830-1230-1 | 9.09 | 8072 ± 44 | 3.13 ± 0.03 | –1.5 | −1.48 ± 0.06 | 11 | 1 |
| HD 74721 | 816-2644-1 | 8.70 | 8908 ± 88 | 3.31 ± 0.02 | –1.5 | −1.41 ± 0.04 | 2 | 1 |
| HD 78913 | 9195-1020-1 | 9.28 | 8515 ± 355 | 3.25 ± 0.01 | –1.5 | 14 | 1 | |
| HD 86986 | 835-1408-1 | 7.98 | 7936 ± 47 | 3.19 ± 0.03 | –1.5 | −1.85 ± 0.05 | 4 | 1 |
| HD 87047 | 2503-1098-1 | 9.72 | 7828 ± 49 | 3.07 ± 0.04 | –2.5 | −2.36 ± 0.10 | 0 | 1 |
| HD 87112 | 3821-809-1 | 9.70 | 9733 ± 38 | 3.48 ± 0.01 | –1.5 | −1.65 ± 0.07 | 3 | 1 |
| HD 93329 | 849-785-1 | 8.77 | 8237 ± 82 | 3.12 ± 0.05 | –1.5 | −1.49 ± 0.08 | 7 | 1 |
| HD 106304 | 7760-1284-1 | 9.06 | 9747 ± 365 | 3.50 ± 0.03 | –1.5 | 10 | 1 | |
| HD 109995 | 3018-494-1 | 7.59 | 8514 ± 123 | 3.08 ± 0.07 | –1.5 | −1.76 ± 0.09 | 25 | 1 |
| HD 117880 | 6125-410-1 | 9.06 | 9285 ± 131 | 3.34 ± 0.09 | –1.5 | −2.25 ± 0.14 | 13 | 1 |
| HD 128801 | 911-1261-1 | 8.73 | 10 313 ± 163 | 3.55 ± 0.02 | –1.5 | −1.38 ± 0.09 | 4 | 1 |
| HD 130095 | 6754-156-1 | 8.14 | 9010 ± 90 | 3.30 ± 0.03 | –2.0 | 5 | 1 | |
| HD 130201 | 8279-2-1 | 10.06 | 8645 ± 275 | 3.48 ± 0.03 | –1.5 | 16 | 1 | |
| HD 139961 | 7849-447-1 | 8.84 | 8517 ± 83 | 3.23 ± 0.07 | –1.5 | 39 | 1 | |
| HD 161817 | 2081-3673-1 | 6.98 | 7533 ± 10 | 3.00 ± 0.01 | –1.5 | −1.52 ± 0.05 | 17 | 1 |
| HD 167105 | 3536-45-1 | 8.94 | 9025 ± 111 | 3.29 ± 0.04 | –1.5 | −1.62 ± 0.08 | 21 | 1 |
| HD 180903 | 6879-187-1 | 9.57 | 7683 ± 44 | 3.10 ± 0.01 | –1.5 | −1.73 ± 0.08 | 17 | 1 |
| HD 213468 | 8003-27-1 | 10.81 | 9147 ± 68 | 3.28 ± 0.02 | –1.5 | 12 | 1 | |
| HD 252940 | 1885-326-1 | 9.08 | 7563 ± 37 | 2.95 ± 0.05 | –1.5 | −1.70 ± 0.09 | 24 | 1 |
| HZ 27 | 12.81 | 9883 ± 289 | 3.38 ± 0.49 | −1.39 ± 0.35 | 7 | 2 |
Notes. The [M/H] values are according to Kinman et al. (2000) whereas [Fe/H] is taken from Behr (2003). The V magnitudes are from Kharchenko (2001).
References. 1: Kinman et al. (2000), 2: Behr (2003).
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