Rotation curves of the Fermionic-MW model (this work, in dashed amber) and the NFW-MW model (Malhan & Ibata 2019, in dotted green), which fit the GD-1 stream, are compared a posteriori with different observed rotation curves (Eilers et al. 2019 with purple triangles, Sofue 2020 with light blue rhombi, and Jiao et al. 2023 with black circles). Only the Fermionic MW model can account for the GD-1 stream data and the sharp drop of the recent Gaia DR3 rotation curve.