yields. Quantitative solutions rely on the accuracy of the progenitor models, an active area of research.

Results
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In this section we examine the trends in isotopic production of several radioactive isotopes as probes of the supernova explosion energy and/or the progenitor structure. Though none of these isotopes can be taken as pure probes of the supernova parameters, the strong trends observed may prove useful in better understanding the supernova engine when compared to gamma-ray observations. We find that the isotopes that are strong indicators of explosion energy are , , , , and , those that are dependent on the progenitor structure are , , and , and those that probe neither are , , , and . Finally, at the end of the section we briefly discuss the full set of yields produced as a result of this study, which will be made publicly available.

We have focused our study on radioactive isotopes whose decay lines could be of interest for detectability with future $\gamma$-ray missions. We focus on the isotopes listed in @Fryer2019 and their daughter products as potential isotopes that may be observed in nearby supernovae with next generation gamma-ray detectors: , , , , , 