X-Shooting ULLYSES: Massive stars at low metallicity - XIV. Properties of SMC late-O and B supergiants reveal the metallicity dependence of winds in the Magellanic Clouds

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Fig. F.1

Comparison of our obtained parameters to literature values. a: T_eff comparison, b: log g comparison, c: L_bol comparison, d: log $\dot{M}$ $Mathematical equation: ${\dot M}$$ comparison, e: log ${\dot{M}}_{smooth}$ $Mathematical equation: ${{\dot M}_{{\rm{smooth}}}}$$ comparison. Pink triangles: comparison to Backs et al. (2024). Green squares: comparison to Bernini-Peron et al. (2024). Blue Xs: comparison to Trundle et al. (2004) and Trundle & Lennon (2005). Grey diamonds: comparison to values obtained from LIME Sundqvist et al. (2025).

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