Table 4
Atmospheric parameters of the programme stars.
| Star names | Teff | log g | [Fe/H] | Reference |
| (K) | (cm s-2) | (dex) | ||
|
|
||||
| HE 0310+0059 | 4489a/4861 | 1.69 | −1.32 | 1 |
| HE 0518-2322 | 4680a | – | – | – |
| HE 0519-2053 | 4775 | 1.46 | −1.45 | 1 |
| HE 0915-0327 | 2920a | – | – | – |
| HE 0916-0037 | 4872a | – | – | – |
| HE 1030-1518 | 4350a | – | – | – |
| HE 1056-1855 | 4280a | – | – | – |
| HE 1345-2616 | 4233a | – | – | – |
| HE 1428-1950 | 4531 | 0.85 | −2.07 | 1 |
| HE 1429-1411 | 3058a | – | – | – |
| HD 55496 | 4800 | 2.8 | –1.55 | 2 |
| HD 81192 | 4705 | 2.50 | –0.62 | 2 |
| 4582 | 2.75 | –0.70 | 3 | |
| 4755 | 2.4 | –0.60 | 4 | |
| 4755 | 2.4 | –0.61 | 5 | |
| HD 92545 | 6240 | 4.23 | –0.26 | 6 |
| HD 100764 | 4846 | 2.2 | –0.59 | 7 |
| LEE 107 | 3288a | – | – | – |
| HD 107574 | 6340 | 3.87 | –0.36 | 6 |
| 6340 | 3.87 | –0.54 | 6 | |
| 6340 | 3.87 | –0.16 | 6 | |
| HD 111721 | 4995 | 2.52 | –1.26 | 8 |
| 4825 | 2.2 | –1.54 | 9 | |
| 4800 | 3.00 | –1.68 | 10 | |
| 5164 | 3.27 | –0.98 | 11 | |
| 4940 | 2.40 | –1.34 | 12 | |
| 5103 | 2.87 | –1.25 | 13 | |
| 5000 | –1.34 | 14 | ||
| 4860 | 2.2 | –1.57 | 15 | |
| HD 112869 | 3545a | – | – | – |
| HD 121447 | 4200 | 0.8 | 0.05 | 16 |
| HD 125079 | 5300 | 3.50 | –0.16 | 17 |
| 5305 | 3.50 | –0.30 | 18 | |
| HD 126681 | 5450 | 4.5 | –1.25 | 9 |
| 5533 | 4.2 | –1.14 | 19 | |
| 5595 | 4.43 | –1.12 | 20 | |
| 5625 | 4.95 | –1.09 | 11 | |
| 5500 | 4.63 | –1.45 | 21 | |
| HD 164922 | 5412a | – | – | – |
References. 1) Kennedy et al. (2011); 2) Cennaro et al. (2007); 3) Cottrell & Sneden (1986); 4) Luck & Bond (1985); 5) Luck & Bond (1983); 6) North et al. (1994); 7) Dominy (1984); 8) Gratton & Sneden (1994); 9) Fulbright (2000); 10) Cavallo et al. (1997); 11) Gratton et al. (1996); 12) Ryan & Lambert (1995); 13) Gratton & Sneden (1994); 14) Pilachowski (1993); 15) Francois (1988); 16) Smith (1984); 17) Smith et al. (1993); 18) Smith & Lambert (1986); 19) Nissen et al. (2000); 20) Nissen & Schuster (1997); 21) Tomkin et al. (1992);
estimated from (J−K) temperature calibrations of Alonso et al. (1996).
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