The eROSITA Final Equatorial-Depth Survey (eFEDS) - X-ray observable-to-mass-and-redshift relations of galaxy clusters and groups with weak-lensing mass calibration from the Hyper Suprime-Cam Subaru Strategic Program survey

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

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Fig. 9

Cluster mass M₅₀₀ and redshift z of each cluster color coded by the quantity f_cont. The mass is randomly sampled from the posterior of M₅₀₀ as an ensemble mass (see Eq. (66)).

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