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Table 2

Typical abundance uncertainties for the disk and bulge stellar samples.

Uncertainty Sc V Cr Mn Co Ni Component
σparam (dex) 0.07 0.1 0.08 0.03 0.05 0.06 Disk
0.1 0.2 0.1 0.06 0.1 0.1 Bulge

σlbl (dex) 0.01 0.08 0.09 0.06 0.05 0.05 Disk
0.04 0.08 0.2 0.1 0.06 0.1 Bulge

σtotal (dex) 0.07 0.1 0.1 0.07 0.06 0.06 Disk
0.2 0.2 0.2 0.1 0.1 0.1 Bulge

Notes. σparam is the uncertainty due to the changes in the stellar parameters using the FIES spectrum of αBoo; σlbl is the uncertainty derived from the line-by-line abundance scatter for each element using the FIES spectrum of αBoo (disk) and B3-f1 (bulge); and σtotal is the combined uncertainty, as in Eq. (1).

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