Fig. B.1.
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X-ray luminosity L2 − 10 keV as a function of the AGN contribution to the far-IR emission. The symbols represent our sample at z ∼ 1.2 and are color coded according to fAGN as in previous figures. The arrow marks the floor of fAGN = 1% adopted in this work. The solid orange star indicates the object from Brusa et al. (2018), which is part of our parent sample.
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