Comparison between the trend of overshoot with stellar mass for models in this paper and that reported by Claret & Torres (2017) and Claret & Torres (2018). The dotted lines show the range of overshoot found to be acceptable solutions for all systems in this study (and where members of each pair have the same overshooting parameter and MLT mixing length parameters. The square symbols show the best fits from Claret & Torres (2017) using the A09 mixture.
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