Table 3: Final (averaged) abundances and uncertainties with [Fe/H] data from previous studies. For the latter data, uncertainties (where available) are given in parentheses.
Star [Fe/H] $\sigma$ [Fe/H]1 [Fe/H]2 [Fe/H]3 [Fe/H]4
  (dex) (dex) (dex) (dex) (dex) (dex)
Y Car -0.05 0.16 -0.33 (0.35) - - -
EY Car -0.17 0.22 - - - -
GZ Car -0.07 0.20 -0.36 (0.33) -0.08 - -
UZ Cen -0.19 0.17 -0.30 (0.32) -0.09 - -
BK Cen 0.07 0.19 -0.03 (0.30) - - -
VX Pup -0.20 0.14 -0.39 (0.14) -0.17 -0.13 -0.15 (0.12)
EW Sct -0.01 0.18 -0.08 (0.09) - +0.03 -
V367 Sct 0.075 0.21 +0.26 (0.30) - -0.01 -
V458 Sct 0.09 0.18 - - - -
BQ Ser -0.13 0.24 -0.36 (0.20) -0.08 -0.05 -
U TrA -0.15 0.16 -0.31 (0.34) - - -
AP Vel -0.06 0.18 -0.18 (0.35) -0.045 - -
AX Vel -0.09 0.18 -0.43 (0.29) -0.12 - -0.15 (0.07)
GSC 8607-0608 -0.11 0.22 - - - -
GSC 8691-1294 -0.015 0.22 - - - -
TU Cas -0.16 0.24 -0.43 (0.31) -0.05 0.02 -
V1048 Cen -0.18 0.22 - - - -
References to [Fe/H] values: 1: Andrievsky et al. (1994); 2: D'Cruz et al. (2000);
3: Andrievsky et al. (2002); 4: Lemasle et al. (2007).

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