Table 1: List of observed stars in the visible, with the values of the parameters taken from the mean-values listed by Gray (1992) and Schmidt-Kaler (1982) or from (1) Nordström et al. (2004); (2) Cayrel de Strobel et al. (2001); and (3) Barbuy & Grenon (1990). In the last column, when no information is available on metallicity, a dash replaces it. The quantity $\langle v\sin i\rangle $ is given in km s-1.
Name Spectral type $\langle v\sin i\rangle $ $T_{\rm eff}$(K) log g [Fe/H]
HD 116608, HD 190785, HD 124320 A1-3 V 145 8900 4.2 -
& HD 221741          
HD 88815 F2 V 90 72441 4.3 -0.131
HD 187691, HD 149890 F8-9 V 7 60261, 59021 4.4 0.072, -0.441
HD 121370 rG0 IV 5 59571 4.4 +0.272
HD 38858 G4 V 3 56361 4.5 -0.261
HD 161797 rG5 IV 3 5700 4.5 +0.232
HD 149661, HD 151541, HD 33278, G9K0 V 2 51761, 52361, 5300, 4.5 0.011, -0.361, -
HD 23524, SAO 66004, SAO 84725     52001, 5300, 5300   -0.491, -, -
HD 93800 rK0 V 2 5250 4.5 +0.433
HD 39715 rK3 V 1 4850 4.6 +0.333
HD 36395 rM1 V 1 3850 4.6 +0.62
HD 15866, HD 25894, HD 2506 G0-4 III 10 5500 3.0 -
HD 163993 wG8 III 3 4950 2.7 -0.12
HD 72324 G9 III 3 4900 2.7 -
HD 33506, HD 112989 rG9K2 III 2 4700 2.6 +0.142
SAO 76803 K2 III 2 4500 2.5 -
HD 181984 rK2 III 2 4500 2.5 +0.12
HD 176670 rK3 III 1 4300 2.2 -0.032
HD 154733, HD 21110 K4 III 1 4000 2.0 -0.142, -


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