Uncertainties in the derived abundances due to typical variations (or uncertainties) in the stellar parameters for a typical star with Teff = 3700 K, log g = 1.5, ξmicro = 2.0 km s-1, and solar metallicity.
|Uncertainty||δ [ Fe / H ]||δ [ Mg / Fe ]||δ [ Si / Fe ]||δ [ Ca / Fe ]|
|δTeff = + 150 K||+0.02||−0.02||−0.10||+0.07|
|δlog g = + 0.5||+0.02||−0.02||± 0.00||− 0.01|
|δ [ Fe / H ] = + 0.1||−0.08||−0.09||−0.08|
|δξmicro = + 0.5||−0.10||−0.07||−0.03||+0.06|
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