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. 2

Observed count rate η (in the unit of counts per second) and the redshift z of the 542 eFEDS clusters. The 434 secure clusters with f_cont < 0.2 (see Sect. 2.3) are shown as the circles, while the rest are marked by red triangles.

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