The yields of each metal from each astrophysical source in the simulation. The shaded regions include the yield range for progenitor stars at different metallicities for a given progenitor mass. AGB wind yields are from S. Cristallo et al. (2015), SN Ia yields are from F.-K. Thielemann et al. (1986), Population II CCSN and massive-star wind yields are from M. Limongi & A. Chieffi (2018), and Population III yields are from A. Heger & S. E. Woosley (2010).