Fig. 3
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Similar to Fig. 2, richness vs. redshift plot for eFEDS J092739.7-010427 for four MCMF runs. The runs using LS (red and green) both show a clear cluster peak and agree well with one other. The MCMF runs using HSC S19A data (black) and S20A data (blue) show a significantly smaller peak due to local offsets in the photometric zeropoint.
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