Fig. D.3.
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To investigate the impact of image separation on classification, we divide the LSNe Ia systems into three bins based on Einstein radius: 0.5″ ≤ θE < 1.0″, 1.0″ ≤ θE < 1.5″, and 1.5″ ≤ θE < 2.0″. The four panels show the distributions of predicted scores (𝒫) for these three subsets after the 1st, 3rd, 7th, and 14th observation epochs, respectively.
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