Observed weak-lensing RAR for ETGs and LTGs from Brouwer et al. (2021) with the stellar M/L_* corrected to use the same stellar population model as the observed kinematic RAR (McGaugh 2022, priv. comm.) relative to the MOND prediction. This does not include the hot gas estimate from Brouwer et al. (2021). Here, we take a_MOND = a_bν_e(a_b/a₀) with (Lelli et al. 2017). Data points below a_b = 10⁻¹³ m s⁻² are shown in white since the isolation criterion is less reliable there (Brouwer et al. 2021).