The left panel is a histogram of the number of stars per bin (on a log scale) with stacked bars of the original truncated metal-poor tail of APOGEE with weighted metallicities from the high-confidence sample. The reported metallicities already include the quality cuts. On the right, the same clean sample with weighted metallicities is mapped onto the celestial sphere and superimposed on the APOGEE footprint. The location of the LMC and SMC, where there is a concentration of stars, has been marked.