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Table 4:

Parameters of the stars (Col. 1) obtained with MA$\chi $ for both types of analysis discussed in the text.
  MA$\chi $, free MA$\chi $, restr. Classical, EW
Star ${T_{\rm eff}}$ (K) $\log g$ [Fe/H] ${T_{\rm eff}}$ (K) $\log g$ [Fe/H] ${T_{\rm eff}}$ (K) $\log g$ [Fe/H] vt (km s-1)
HD 3567 6103.5 4.79 -1.200 6176.0 4.20 -1.223 6035.0 4.08 -1.200 1.50
HD 19445 - - - 5746.5 4.10 -2.293 5982.0 4.38 -2.075 1.40
HD 22879 5770.6 4.31 -0.877 5778.1 4.31 -0.880 5792.0 4.29 -0.885 1.20
HD 25704 5638.9 3.61 -1.094 5864.4 4.19 -0.912 5700.0 4.18 -1.010 1.00
HD 63077 5795.5 4.21 -0.796 5787.7 4.21 -0.793 5629.0 4.15 -0.935 0.90
HD 63598 6078.6 4.79 -0.681 5804.1 4.23 -0.901 5680.0 4.16 -0.885 0.90
HD 97320 5601.1 4.65 -1.411 6025.1 4.24 -1.183 6105.0 4.18 -1.175 1.20
HD 103723 5999.2 4.29 -0.896 6004.4 4.29 -0.896 6128.0 4.28 -0.805 1.50
HD 105004 5802.5 4.33 -0.900 5802.5 4.33 -0.900 5900.0 4.30 -0.800 1.10
HD 106038 5994.6 4.48 -1.392 5995.5 4.48 -1.392 5950.0 4.33 -1.390 1.10
HD 113679 6037.3 4.73 -0.500 5757.5 4.35 -0.708 5759.0 4.04 -0.590 0.90
HD 116064 5757.7 4.58 -2.41 5757.7 4.58 -2.401 5999.0 4.33 -2.000 1.50
HD 121004 5509.2 4.05 -0.670 5657.8 4.40 -0.650 5711.0 4.46 -0.725 0.65
HD 122196 5811.8 3.50 -1.954 5810.2 3.56 -1.954 6048.0 3.89 -1.760 1.20
HD 126681 5556.9 4.44 -1.055 5521.6 4.68 -1.075 5532.0 4.58 -1.170 0.60
HD 160617 5804.1 3.50 -1.961 5985.2 3.75 -1.794 6028.0 3.79 -1.785 1.30
HD 175179 6080.5 5.00 -0.500 5779.5 4.47 -0.691 5758.0 4.16 -0.690 0.90
HD 188510 5568.8 4.35 -1.341 5500.0 4.65 -1.231 5536.0 4.63 -1.600 1.00
HD 189558 5610.8 3.58 -1.191 5500.0 3.75 -1.181 5712.0 3.79 -1.145 1.20
HD 195633 6318.2 4.61 -0.500 6037.7 3.99 -0.687 6005.0 3.86 -0.625 1.40
HD 205650 5693.7 4.93 -1.195 5754.0 4.47 -1.208 5842.0 4.49 -1.170 0.90
HD 298986 5891.5 3.66 -1.592 6297.9 4.22 -1.304 6144.0 4.18 -1.410 1.40
CD-333337 5808.2 3.66 -1.598 5946.9 3.85 -1.490 5952.0 3.95 -1.435 1.40
CD-453283 5500.0 4.26 -0.978 5885.5 5.00 -0.685 5657.0 4.97 -0.835 0.80
CD-571633 5939.9 4.37 -0.893 5939.9 4.37 -0.893 5907.0 4.26 -0.930 1.10
CD-3018140 6143.1 3.50 -2.095 6246.5 3.50 -1.980 6340.0 4.13 -1.870 1.00
G005-040 6228.2 5.00 -0.584 5930.4 4.52 -0.794 5766.0 4.23 -0.840 0.80
G013-009 6529.5 4.58 -2.29 6556.0 4.08 -2.299 6416.0 3.95 -2.225 1.40

Notes. In the first analysis all three parameters are determined with only the spectrum, while in the second one $\log g$ was determined independently by using parallaxes according to Eq. (14), as for the classical method (EW; last four columns).




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