Our α _ov,eff vs. stellar mass results (red points) in comparison with other studies of convective core overshoot, including those shown in Figure 7 as well as the eclipsing binary work of Claret & Torres (2018) and Claret & Torres (2019), shown in black triangles. The machine-learning results for γ Doradus stars from Mombarg et al. (2021) are shown in maroon triangles.