Abundance uncertainties due to stellar parameters.
|A: Teff = 5750, log g = 3.7 dex, vt = 1.4 km s-1|
|B: Teff = 5750, log g = 3.6 dex, vt = 1.4 km s-1|
|C: Teff = 5750, log g = 3.7 dex, vt = 1.3 km s-1|
|D: Teff = 5650, log g = 3.7 dex, vt = 1.4 km s-1|
|E: Teff = 5650, log g = 3.3 dex, vt = 1.2 km s-1|
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