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. 10

Observed count rate 77 as a function of the cluster mass M₅₀₀ (left panel) and redshift z (right panel). The circles in the left and right panels represent the measurements of η color-coded by the cluster redshift and mass, respectively. The gray shaded regions are the best-fit models. In the left (right) panel, we normalize the observed count rate to that at the pivotal redshift z_piv = 0.35 (pivotal mass M_piv = 1.4 × 10¹⁴h⁻¹M_⊙).

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