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Fig. 8.

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Radio loudness as a function of the α ox $ \tilde{\alpha}_{\mathrm{ox}} $ parameter for the objects presented in this work (blue circle, red square, and green upper limit) as well as for a complete radio-selected sample of z > 4 blazars (Caccianiga et al. 2019; Ighina et al. 2019) and z > 4 radio QSOs from the literature (Caccianiga et al. 2024, black points, and from single studies, pink symbols; see Table A.1). The shaded grey regions at α ox 1.35 $ \tilde{\alpha}_{\mathrm{ox}}\sim1.35 $ and log(R)∼2 divide the parameter space in two main regions: X-ray-, radio-bright objects (top-right corner, likely blazars) and X-ray-, radio-faint objects (bottom-left corner, likely hosting mis-aligned jets, i.e., classic RL QSOs).

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