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Fig. A.1.

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Evolutionary tracks of 5 M stellar models with LMC-like (left) and SMC-like (right) metallicities. The solid blue, dashed orange and dotted purple lines denote our MESA models, the SYCLIST models, and the MIST models, respectively. The adopted metallicity Z in different model sets are listed in the legend. In each model set, stellar evolutionary tracks from left to right correspond to models with increasing initial rotational velocity, with values listed in the legend. Numbers in the parentheses indicate the formally labeled fractional critical angular velocities in the SCYLIST web interface.

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