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Fig. A.1

image

Core-collapse supernova rate as a function of time in a population of single stars (top) and a realistic mix of single stars and binaries (bottom) formed as an instantaneous starburst at t = 0, for our standard assumptions. The red dashed lines show the fitting formulae. The top axis shows the initial mass of single stars with the corresponding lifetime given in the bottom axis, computed with binary_c.

This figure is made of several images, please see below:

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