Table 7: Oxygen abundance comparison with Takeda (2003).
Star $T_{\rm eff}$   [Fe/H]   $\log \epsilon$(O)   [O/Fe $]_{\rm NLTE}$
  TW T03   TW T03   TW T03   TW T03
HD 108177 6036 5960    -1.69  -1.87   7.79 7.84   0.65 0.78
BD +02$^{\circ }$3375 5926 5800    -2.25  -2.40   7.17 7.51   0.59 0.98
BD +20$^{\circ }$3603 6138 6020    -2.09  -2.17   7.48 7.40   0.66 0.72
BD +26$^{\circ }$2606* 6086 5980    -2.27  -2.40   7.24 7.67   0.68 1.14
BD +29$^{\circ }$2091 5648 5630    -1.96  -2.20   7.43 7.71   0.56 0.98
BD +34$^{\circ }$2476 6247 6120    -1.94  -2.19   7.49 7.52   0.60 0.78
BD +51$^{\circ }$1696 5537 5600    -1.48  -1.49   7.88 8.15   0.53 0.71
TW: This work; T03: Takeda (2003).
 $\ast$ : For this star the reanalysis data used by Takeda is from Abia & Rebolo (1989),
and remaining stars' data are from Tomkin et al. (1992).

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