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Table 5:

1D Fe abundances for six stars in the sample of Israelian et al. (1998,2001), from three Fe I lines of different excitation potentials.

Star
$T_{\rm eff}\;$ $\log{g}\;$ $\xi_t$ [Fe/H] [Fe I/H]3143 [Fe I/H]3149 [Fe I/H]3152
  [K] [dex] [ ${\rm km}\:{\rm s}^{-1}\;$] [dex] [dex] [dex] [dex]

G 64-12
6318 4.20 1.0 -3.37 -3.44 -3.38 -3.43
G 64-37 6310 4.20 1.0 -3.22 -3.22 -3.21 -3.19
LP 815-43 6265 4.54 1.0 -3.05 -3.06 -2.92 -3.05
HD 140283 5550 3.35 1.0 -2.70 -2.77 -2.57 -2.83
HD 166913 5965 3.90 1.0 -1.80 - -1.57 -1.78
HD 76932 5800 3.85 1.0 -1.10 - -1.48 -1.45


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