Fig. C.1.
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Histograms of the magnitude residuals between LS and DES photometry (Δ = mLS − mDES) for the 8,412 galaxies in our sample that passed the quality cuts. Each panel corresponds to one photometric band: g (top left), r (top right), i (bottom left), and z (bottom right). The median and standard deviation of the residuals in each band are indicated within the corresponding panel. The small offsets confirm the overall consistency between both surveys.
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