Selection function of clusters in Dark Energy Survey year 3 data from cross-matching with South Pole Telescope detections
Context. Galaxy clusters selected based on overdensities of galaxies in photometric surveys provide the largest cluster samples. However, modeling the selection function of such samples is complicated by noncluster members projected along the line of sight (projection effects) and the potential detection of unvirialized objects (contamination)
Grandis, S. et al.
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2025