Table 3: Errors in the abundances of Star # 1282 due to uncertainties in the atmospheric parameters.
  $\Delta A$(Fe I) $\Delta A$(Fe II) $\Delta A$(Mg) $\Delta A$(Si) $\Delta A$(Ca) $\Delta A$(Ti) $\Delta A$(Ni)
$\Delta \xi = \pm 0.2$ km s-1 $^{\rm -0.07}_{+0.08}$ $^{\rm -0.05}_{+0.04}$ $^{\rm -0.03}_{-0.04}$ $\mp 0.03$ $^{\rm -0.12}_{+0.13}$ $^{\rm -0.09}_{+0.10}$ $\mp 0.07$
$ \Delta T_{\rm eff} = \pm 100$ K $^{\rm +0.01}_{+0.00}$ $^{\rm -0.15}_{+0.16}$ $^{\rm +0.03}_{+0.00}$ $^{\rm -0.08}_{+0.11}$ $^{\rm +0.11}_{-0.12}$ $^{\rm +0.18}_{-0.17}$ $^{\rm +0.00}_{-0.01}$
               
$\Delta T_{\rm eff} = \pm 100~K~~\Delta \log~ g = \pm
0.20$ $^{\rm +0.07}_{-0.04}$ $^{\rm +0.03}_{+0.04}$ $^{\rm +0.04}_{-0.02}$ $^{\rm +0.00}_{+0.04}
$ $\pm 0.11 $ $\pm 0.019 $ $^{\rm +0.08}_{-0.05}$
               
$\Delta \log g = \pm 0.50 $ $^{\rm +0.09}_{-0.10}$ $^{\rm +0.24}_{-0.30}$ $^{\rm +0.04}_{-0.03}$ $^{\rm +0.12}_{-0.14}$ $^{\rm -0.01}_{+0.00}$ $^{\rm +0.02}_{-0.03}$ $^{\rm +0.11}_{-0.13}$


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