RAR for different baryonic masses and boundary conditions for numerical solutions with f_G/m² = 0.99 Mpc². The solid lines are for boundary conditions where stays within a fraction δ = 0.1 from MOND up to the largest possible radius for a given baryonic mass M_b. Dash-dotted and dashed lines correspond to these optimal boundary conditions multiplied by factors [0.8, 0.9] and [1.2, 1.4], respectively. The dips all go to −∞ since they correspond to M_eff = 0 (i.e., a_tot = 0), but this is not resolved numerically. The y-axis shows the modulus of a_tot. So after the dip, the direction of the accelerations is flipped. All solutions are cut off where the condensate density of the largest boundary-condition solution for a given M_b first drops to zero. The observed weak-lensing RAR does not include the hot gas estimate of Brouwer et al. (2021). We correct the observed weak-lensing RAR to be consistent with the M/L_* scale of the observed kinematic RAR (McGaugh, priv. comm.). Data points below a_b = 10⁻¹³ m/s² have a lighter color since the isolation criterion is less reliable there (Brouwer et al. 2021).