Fig. 15.
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One- and two-dimensional marginal contour plots for the WL mass calibration of the eROSITA count rate to halo mass relation. In green the results from KiDS-1000 on eRASS1 are shown, in blue are the results from DES Y3 on eRASS1 (Grandis et al. 2024), in orange are the results from HSC-Y3 on eRASS1, and in black are the results from HSC-Y3 on eFEDS (Chiu et al. 2022). All results show agreement, indicating the reliability of the WL mass calibration methods employed by the different teams.
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