MADNESS deblender - Maximum A posteriori with Deep NEural networks for Source Separation

Open Access

Fig. 13

Distribution of ellipticity residuals for the deblended models of MADNESS, SCARLET, and VAE-deblender in the r-band of galaxies from the TestFields in different bins of e₁ (top) or e₂ (bottom). The boxes and whiskers in the plot indicate the ranges from 25^th to 75^th and 5^th to 95^th percentiles, respectively.

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