Evaluation of the effectiveness of the correction functions in reproducing the intrinsic concentration and asymmetry. The top two rows present comparisons of the concentration measured from simulated CEERS images (C), bias-corrected values (C_cor), and intrinsic values (C_True). The bottom two rows illustrate comparisons of asymmetry measured from simulated CEERS images using the conventional method (A_C00), bias-corrected values (A_cor), and intrinsic values (A_True). Columns one through four show results for z = 0.75, 1.5, 2.25, and 3.0, respectively. The mean difference (Δ) and scatter (σ) between the y-axis and x-axis values are indicated at the top of each panel. In the A_True − A_cor relations, data are divided into two groups: angularly small galaxies with R_p, True/FWHM < 5 (red circles) and angularly large galaxies with R_p, cor/FWHM ≥ 5 (blue crosses).