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. 10

Kinetic luminosity of BCG radio galaxies estimated at 1.4 GHz vs. X-ray luminosity of the host cluster or group for the eFEDS (blue) and P20 (red) samples. The black line represents the best-fit estimated from Bayesian inference: log L_kin = (1.07 ± 0.11)log L_X−(2.19 ± 4.05). The grey area indicates 1σ errors.

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