Predicted solar elemental distribution normalized to the solar abundances of Asplund et al. (2009). The blue bars show our chemical evolution prediction when combining the contribution of CC SNe (top: Limongi & Chieffi 2018, bottom: Nomoto et al. 2013), low- and intermediate-mass stars (Cristallo et al. 2015), and SNe Ia (using the metallicity-dependent yields from this work). The orange bands show the specific contrition of SNe Ia within the combined predicted abundances.