Vecolity offset, ΔK_p, as a function of different stellar masses. This plot serves to visualise the Table 6 in comparison with global circulation model predictions. Each data point with uncertainties corresponds to the computed ΔK_p as a function of the stellar mass (reported in Table 6) as derived by Delrez et al. (2016) (M_⋆ = 1.35 ± 0.08 M_⊙), Borsa et al. (2021) (M_⋆ = 1.38 ± 0.02 M_⊙), Sing et al. (2024) (M_⋆ = 1.33 ± 0.02 M_⊙), and Prinoth et al. (2025) (M_⋆ = 1.42 ± 0.03 M_⊙), respectively. Uncertainties are calculated via error propagation. Vertical lines mark the GCM predictions, namely models with zero, weak, and strong drag by Tan et al. (2024) and drag-free models by Parmentier et al. (2018).