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. 4

Distribution of offsets between the X-ray and optically defined centers of eFEDS clusters. The blue histogram is the observed offset distribution in the unit of the scale radius. The black solid line represents the best-fit model, i.e., Eq. (20), which consists of centering and mis-centering components, as indicated by the red and green dashed lines, respectively.

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