those that may be of use for the next generation of gamma-ray astronomy.

The nucleosynthetic yields presented in @Fryer_2018 were produced by post-processing the explosive trajectories with the publicly-available version of the Torch nuclear reaction network [@Timmes_2000] using the initial abundances from the stellar evolution results (which included only a small number of isotopes). This effort focused on general trends (production of Fe, Si, C, O, Ar, S, Ca, Ne, Mg) in the explosive yields. Here, we extend this past work, using the NuGrid nuclear network to post-processes both the stellar evolution as well as the explosive trajectories. We focus the study of this paper on the detailed NuGrid yields of several radioactive nuclei of interest that are produced in core-collapse supernovae, and their dependence on explosion energy and progenitor structure. We then comment on the observational prospects of these isotopes to be compared to sensitivities of next generation of gamma-ray telescopes.

The structure for the remainder of this paper is as follows. Section \[methodology\] examines the methodology employed in this study; particularly, the initial abundances, explosion parameterization, and nuclear reaction network used. Section \[results\] discusses the effect of the parameters on general burning trends and on a set of 