The features of single star models in grid CC-S at the end of the run. The middle panel shows the final mass (black), He-core mass (blue) and CO-core mass (green). The bottom panel shows the surface composition (solid lines, left axis) and the central C abundance at core He-depletion (dotted line, right axis). The top panel highlights the models that are expected to implode (black background), for different explodability criteria. Background colors show the expected evolutionary outcome of a model in that mass range, either WD (white), Type IIP/L (red), Type IIb (green) or Type Ibc supernova (blue).