Theoretical Observables of 3D Core-Collapse Supernova Simulations

We have completed many state-of-the-art 3D simulations of core-collapse supernovae (CCSNe) and we are now extracting a suite of observables and the systematics with the progenitor mass. In this talk I will present many new results concerning the explodability of progenitor massive stars, among which are the nucleosythetic yields as a function of progenitor and the gravitational wave signatures.