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Fig. 9

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Aperture-photometry results in the r-band of galaxies from TestFields after deblending with MADNESS, SCARLET, in terms of signal-to-noise ratio (S/N), blendedness (β), and contamination (κ) in the r-band. In each panel, the top plot shows the distribution of the absolute value of relative flux residual (∣δ F/F∣) while the bottom plot shows the distribution of galaxies for the metric on the x-axis. The boxes in the plot on top show the range from the 25th to 75th percentile, with a horizontal line representing the median, while the whiskers represent the 5th to 95th percentile of relative residuals in the r-band.

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