Filled bigger circles show the abundance results for 25 of the 26 microlensed dwarf and subgiant stars in the Bulge (only stellar parameters were determined for the star from Epstein et al. 2010; that we analysed in Bensby et al. 2010c). Thick disk and thin disk stars from (Bensby et al. 2003, 2005, and in prep.) are shown as small circles red and blue circles, respectively. The error bars represent the total uncertainty in the abundance ratios and have been calculated according to the prescription in Epstein et al. (2010), see Sect. 3.