Fig. 2.

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X-ray luminosity expected from X-ray binaries and hot gas of the GAMA09 matched galaxies versus the intrinsic 2 − 10 keV luminosity of each eFEDS X-ray source, colour coded according to the stellar mass (explained in Sect. 3.1.3). Sources lying above the 1:3 solid black line have X-ray emission securely dominated by AGN processes and constitute our X-ray AGN sample; sources in the shaded area are compatible with non-AGN emission processes, and excluded from the analysis.
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