Bar fraction vs. stellar mass at ɀ = 0.0, ɀ = 0.5, and ɀ = 1.0 in TNG50. The dashed curve indicates the fit to observations given in Erwin (2018). We have taken this curve from Zhao et al. (2020). The binomials errors on the bar fractions are defined using the bar fraction and the number of total disks, i.e., n_disk, in each mass interval bin as $\text{Δ}=\sqrt{\frac{f_{\text{bar\hspace{0.17em}}}\left(1-f_{\text{bar\hspace{0.17em}}}\right)}{n_{\text{disk\hspace{0.17em}}}}}$ (Rosas-Guevara et al. 2022). The curve for ɀ = 0.0 differs slightly from that shown in Fig. 1 of Roshan et al. (2021b), where the condition F ≤ 0.5 was used instead of F ≤ 0.7. The inset plot displays the bar fraction for bars longer than 2 kpc. This plot is useful because very short bars may not be detected in observations.