RAR of the q = 1 galaxies implied by our SFDM fits for the unrestricted fit (left), the fit restricted to the pseudo-MOND limit (|ε|< 5, middle), and the fit restricted to the proper MOND limit (|ε|< 0.4, right). Each panel also shows the RAR implied by MOND with the SFDM-like interpolation function ν_θ and a₀ = 0.87 ⋅ 10⁻¹⁰ m/s², i.e., a_SFDM = a_b ν_θ(a_b/a₀) (dotted gray line) and by Newtonian gravity with no dark matter (dashed gray line). For the |ε|< 0.4 fit we exclude the galaxies that only barely satisfy |ε|< 0.4 and therefore have a bad χ², i.e., we exclude galaxies with ε > 0.38 and χ² > 100.