Fig. A.5.
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Relationship between effective Einstein crossing time (τeff) and lens mass (Mlens) across Galactic components, surveys, and SN engine models. The colour-centre scale is consistent across all panels, revealing three distinct populations of SL systems. The mass gap region (Mlens ∈ [2, 5]) shows the highest population density in the f05 model and the lowest in the f40 model.
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