Same as Fig. 1, but for different mass re-scalings of the Rocha et al. (2012) simulations. In the bottom right of each panel the numbers indicate the predicted time for GCs associated with the bulge, GSE, and Sgr when they are inserted into the m12c halo potential, as well as the probability they can lie in the distribution of subhalos. (Top:) We have scaled down the Rocha et al. (2012) main halo mass to 7.4× 10¹⁰ M_⊙ and add a baryonic component of 6.2× 10¹¹ M_⊙, similar to that used in Jiao et al. (2023) and Ou et al. (2024). (Bottom panel:) We have scaled up the Rocha et al. (2012) main halo mass to 19.4× 10¹⁰ M_⊙, also adding a baryonic mass of 6.2× 10¹¹ M_⊙.