The eROSITA Final Equatorial-Depth Survey (eFEDS) - LOFAR view of brightest cluster galaxies and AGN feedback

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

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Fig. 3

Left: histogram showing the redshift distribution of the sample, classified into radio detections (red) and upper limits (blue). Right: L_X500 vs. redshift for the sample. The dashed line denotes the theoretical flux cut of the eROSITA observation.

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