Fig. 17.
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Fraction of GAMA09 galaxies hosting eROSITA-eFEDS-detected X-ray AGN as a function of λEdd in different stellar mass (yellow, green, teal, blue) and redshift (two panels) bins. The results agree well with those of Aird et al. (2012, black dashed lines), corroborating the idea that there is a mass-invariant triggering and fuelling mechanism at play in X-ray AGN.
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