Fig. 10

[X/Fe] vs. [Fe/H] trends (LTE) determined for the bulge giants in this work: green squares for S/N above 20, green open circles otherwise. For spectra with S/N < 20 the uncertainty in [X/Fe] becomes significantly large (see Jönsson et al. 2017a). Also plotted are bulge giant trends from Barbuy et al. (2013) (open red diamonds), Ernandes et al. (2018) (blue squares), Johnson et al. (2014) (open orange squares), and Schultheis et al. (2017) (black dots), as well as the microlensed bulge dwarfs from Bensby et al. (2017) (purple filled diamonds). The typical uncertainties for our stars are shown as in Fig. 4.
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