Sensitivity of derived abundances to the atmospheric parameters and EWs.
|ΔTeff = 70 (K)||Δlog g = 0.19 (dex)||Δξ = 0.14 (km s-1)||σ EW||σ tot||σ obs|
|Δ [ O/Fe ]||0.04||0.07||0.03||0.04||0.09||0.15|
|Δ [ Na/Fe ]||0.00||–0.07||–0.03||0.04||0.09||0.29|
|Δ [ Mg/Fe ]||0.11||–0.08||–0.07||0.02||0.15||0.16|
|Δ [ Al/Fe ]||0.02||0.04||0.03||0.04||0.07||0.21|
|Δ [ Si/Fe ]||0.04||0.00||–0.02||0.02||0.05||0.03|
|Δ [ Ca/Fe ]||0.08||–0.01||–0.06||0.02||0.10||0.04|
|Δ [ Sc/Fe ]||0.12||0.16||0.10||0.05||0.23||0.05|
|Δ [ Ti/Fe ]||0.00||0.07||–0.04||0.05||0.09||0.07|
|Δ [ Cr/Fe ]||0.14||0.01||–0.10||0.03||0.17||0.07|
|Δ [ Ni/Fe ]||0.13||0.01||–0.08||0.02||0.15||0.08|
|Δ [ Y/Fe ]||0.03||0.07||–0.01||0.06||0.10||0.04|
|Δ [ Ba/Fe ]||–0.09||–0.06||–0.02||0.06||0.13||0.07|
|Δ [ La/Fe ]||0.12||0.14||0.08||0.07||0.21||0.17|
Notes. The sensitivity determination was performed for Star #3. σEW is the error in the measurements. σtot is the squared root of the sum of the squares of the individual errors. σobs is the mean observed dispersion.
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