CDFs of the percentage of stellar mass of the host galaxy that is enriched by the observed GRB-KN sample (p_enrich) at z = 0 (solid blue) and by the full GRB-KN and short GRB sample (solid gray). We show the same for p_enrich 5 Gyr after enrichment (dashed lines). We find that the median p_enrich = 13% for the GRB-KN sample, suggesting that the majority of their r-process will be lost to the CGM or IGM. The median p_enrich for the full sample is 59%. Given that there is a significant fraction of hosts that have ≲50% enrichment, this suggests that not all environments are capable of being strongly enriched from a single event.