Location of the five analyzed fields: B3, BW, B6, BL, and SW. All of these except SW are previously analyzed in, for example, Lecureur et al. (2007). These locations are compared to the COBE/DIRBE outline of the Galactic bulge (Weiland et al. 1994), the locations of the microlensed bulge dwarf stars of Bensby et al. (2013), and the high-resolution sample of the GIBS survey (González et al. 2015). Also shown is the extinction toward the bulge from the BEAM calculator¹ based on González et al. (2011b, 2012) scaled to optical extinction (Cardelli et al. 1989).