Table 5: Errors in the abundances of star # 628 due to uncertainties in the atmospheric parameters.
$\Delta A$ (FeI) $\Delta A$ (FeII) $\Delta A$ (O) $\Delta A$ (MgI) $\Delta A$ (SiI) $\Delta A$ (CaI)

$\Delta\xi = \pm 0.2$ ${\rm km~s}^{-1}$ $\rm ^{-0.06}_{+ 0.07}$ $\rm ^{-0.04}_{+ 0.05}$ $\mp 0.05$ $\mp 0.04$ $\rm ^{-0.03}_{+ 0.04}$ $\rm ^{-0.05}_{+ 0.06}$

$\Delta T_{\rm eff} = \pm 100$ K $\rm ^{+0.14}_{-0.06}$ $\rm ^{-0.06}_{+0.12}$ $\mp 0.01$ $\rm ^{+0.09}_{-0.06}$ $\rm ^{+0.00}_{-0.05}$ $\rm ^{+0.17}_{-0.10}$

$\Delta \log g = \pm 0.50$ $\rm ^{+0.05}_{-0.03}$ $\rm ^{+0.29}_{-0.20}$ $\rm ^{+0.25}_{-0.24}$ $\rm ^{-0.03}_{+0.01}$ $\rm ^{+0.11}_{-0.06}$ $\rm ^{-0.03}_{+0.01}$

**Table 5:** Errors in the abundances of star # 628 due to uncertainties in the atmospheric parameters.
	$\Delta A$ (FeI)	$\Delta A$ (FeII)	$\Delta A$ (O)	$\Delta A$ (MgI)	$\Delta A$ (SiI)	$\Delta A$ (CaI)
$\Delta\xi = \pm 0.2$ ${\rm km~s}^{-1}$	$\rm ^{-0.06}_{+ 0.07}$	$\rm ^{-0.04}_{+ 0.05}$	$\mp 0.05$	$\mp 0.04$	$\rm ^{-0.03}_{+ 0.04}$	$\rm ^{-0.05}_{+ 0.06}$
$\Delta T_{\rm eff} = \pm 100$ K	$\rm ^{+0.14}_{-0.06}$	$\rm ^{-0.06}_{+0.12}$	$\mp 0.01$	$\rm ^{+0.09}_{-0.06}$	$\rm ^{+0.00}_{-0.05}$	$\rm ^{+0.17}_{-0.10}$
$\Delta \log g = \pm 0.50$	$\rm ^{+0.05}_{-0.03}$	$\rm ^{+0.29}_{-0.20}$	$\rm ^{+0.25}_{-0.24}$	$\rm ^{-0.03}_{+0.01}$	$\rm ^{+0.11}_{-0.06}$	$\rm ^{-0.03}_{+0.01}$

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