Upper panel: [Co/Fe] vs. [Fe/H] with the present results in LTE and corrected for NLTE, together with literature data. Lower panel: [Cu/Fe] vs. [Fe/H] with the present results and literature data. Shown are: the present results in LTE (open green circles); present results in NLTE (open magenta circles); Johnson et al. (2014) (filled blue circles); Lomaeva et al. (2019) for the SW field (open cyan circles); Xu et al. (2019) in LTE (open Indian red triangles); Xu et al. (2019) in NLTE (filled Indian red triangles); Ernandes et al. (2018) for bulge globular clusters (open dark orange squares) and chemodynamical evolution models are overplotted; specific star formation rates of 3 Gyr⁻¹, with SNII yields from WW95 (black lines); specific star formation rates of 1 Gyr⁻¹, with SNII yields from WW95 and from Kobayashi et al. (2006) for [Fe/H] < −4.0 (green lines). Models are for distances to the Galactic center of: r < 0.5 kpc (solid lines), 0.5 < r < 1 kpc (dotted lines), 1 < r < 2 kpc (dashed lines), and 2 < r < 3 kpc (dash-dotted lines).