Fig. 15.
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Flux ratio of the contributing Euclid VIS I1 galaxies in the LSST-like total blends. The sub-panels in the left panel show the scatters and the median values of the flux ratios with different matching radii with the horizontal axis showing the LSST-like r-band magnitude of the total blends. The right panel is the corresponding results of the probability distributions normalized using the number of total blends for a matching radius of 2″.
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