Comparison of distance (d) estimates for eclipsing binaries in the LMC (left panel) and the SMC (right panel). The x axis represents distances (d^r) of eclipsing binaries derived from the literature (d^r). The y axis shows distances (d_SBCR) estimated using the SBCR developed in this study (S​_V = (1.230 ± 0.021)(V − K_s)₀ + (2.845 ± 0.048)). The shaded blue area indicates a deviation range of ±3%. The bottom panel illustrates the distribution of relative errors (Δd/d^r = (d_SBCR − d^r)/d^r).