The eROSITA Final Equatorial-Depth Survey (eFEDS) - Catalog of galaxy clusters and groups

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

Open Access

Fig. 5

Detection probability as a function of luminosity L₅₀₀ in the 0.5–2 keV band and redshift ɀ. The data points with error bars are the L₅₀₀ for the clusters with >2σ measurements. Details of the computation of L₅₀₀ are presented in Sect. 5. The white curve shows the flux limit at 1.5 × 10^–14 erg s^–1 cm^–2, corresponding to an average completeness level of ~40%.

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