Ratio of the yields obtained in this work to those obtained in previous studies, each weighted by a Salpeter IMF and subsequently normalized to one. The red line shows the ratio of our yields to the original yields from WH07, for which every star explodes. The cyan line is the same as the red, except that we apply our explodability to the yields of WH07. This means that for the 12, 14, 15, 18, and 100 M_⊙ stars, which do not explode in our simulations, we only include the winds, whereas for the rest we take the full yields from WH07. The green line shows the ratio of our yields to those by C19. The empty circles and the dashed line connecting them indicate elements for which the total yield is less than 10⁻⁷ M_⊙.