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Fig. 1.

image

Left panel: L2 − 10 as a function of vCIV for the WISSH quasars (black circles). We also report hyper-luminous quasars at z = 2 − 3 (C17 sample, blue triangles). Middle panel: intrinsic αOX as a function of vCIV for the WISSH quasars. Red circles indicate X-ray weak sources (see Sect. 3 for details). Right panel: L2500 Å as a function of vCIV. Solid and dashed lines report the best-fit linear relation and 1σ uncertainties on the normalisation for the WISSH-only relations. Dotted line in the left panel reports the best-fit relation with the addition of the C17 sample. Orange lines in the right panel report the best-fit L2 − 10vCIV relation normalised to the mean values of L2500 Å.

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