Comparison of our structural parameters R_eff(g*), μ_eff, and μ₀ with those from ISIB96 for the test sample galaxies. Our original g‐ and r‐band μ_eff and μ₀ were transformed to B‐band magnitudes. The error bars corresponding to the total rms uncertainties of shown differences. Filled circles denote galaxies that according to ISIB96 had parameters derived from CCD photometry (as opposed to photographic plates).