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Fig. F.1

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Cumulative distribution of the absolute value of the relative flux residuals ∣δ F/F∣ before deblending and after deblending with MADNESS, SCARLET, and VAE-deblender, for each LSST band. The results are presented for two cases: (a) all galaxies in TestFields and (b) galaxies in TestFields with S/Nblend ≥ 5.

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