Mass-loss rates from GA best fits. The supergiants are the blue squares, the giants are the orange triangles, and the dwarfs are the green circles. A linear fit to the GA best-fit mass-loss rates for stars with log(L/L_⊙) ≥ 5.0 is shown by the solid line. Theoretical predictions tailored to our best-fit stellar parameters from Vink (Vink et al. 2001), Krtička (Krtička & Kubát 2018), and Leuven (Björklund et al. 2021) are shown in dotted, dash-dotted, and dashed lines, respectively.