-space data points (points with errors) of three of the cored SPARC galaxies shown in the left-hand panel of Fig. 4, compared to the MOND MI curve with g₀ = 1.2 × 10⁻¹⁰ (solid grey), the MOND MI curve with the best-fit value of g₀ for each galaxy (dashed grey), and MOND MG (Brada-Milgrom approximation) curves (points without errors). We note that most uncertainties are small for most cases because the ratios are constructed to reduce systematic uncertainties. Also shown are the χ²/d.o.f. values for the dashed best-fit MOND MI curves.