Fig. 9.
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Median SB X-ray and 1.4 GHz detection fluxes for each of the fields color-coded as labeled in the right panel. The two panels consider tracks for two different levels of AGN obscuration: log NH = 20.5 (left) and log NH = 24.5 (right). In cyan and in magenta we show the typical 0.5 − 2 keV versus 1.4 GHz flux tracks, computed at different redshifts, for an AGN with log Lbol = 43 and log Lbol = 46, respectively.
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