Probability density maps arising from our simulations plotted against observed stellar streams as in Figs. 10–12, but for the case of the Palomar 5 cluster. Model predictions are compared to the tracks available in the galstreams library and those coming from the work by Ibata et al. (2021, red lines), Price-Whelan et al. (2019, yellow-lines), and Starkman et al. (2020, blue lines). Note: proper motions and distances are not available for the Pal5-S20 track.