Dependence of the fraction of bars (f_{bar,  obs}) and effectiveness of detecting bars (η_eff), measured from the simulated CEERS images as a function of redshift (z). The gray diamonds represent the results obtained from the simulated data with the galaxy evolution model, and the pink stars represent those from the data without a model. The error bars denote the uncertainty of f_{bar,  obs}. For the simulated CEERS images, the F115W, F150W, and F200W filters are used for redshift range z = 0.75–1.0, 1.25–1.75, and 2.0–3.0, respectively. The horizontal dashed line represents the f_{bar,  true} of 68% of our sample.