Fig. 3.
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Un-weighted normalised r-band magnitude distributions of the BOSS/eBOSS spectroscopic samples and UNIONS photometric galaxies. We can see that the spectroscopic galaxies from the BOSS/eBOSS surveys fall into the brighter tail of the UNIONS distribution. The galaxies which dominate the lensing signal are comparatively fainter. Note: we could not use our large overlap with LOWZ galaxies as these bright galaxies (r < 20) are mostly absent from our lensing sample due to size cuts.
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