Fig. 12.
Logarithm of EWs as a function of the velocity shift of the CIV emission line for the SUPER sample (diamonds), colour-coded according to the αOX (top), LBol (middle), and λEdd (bottom). Additionally, the SDSS sample from Shen et al. (2011) (contours and grey points) and the WISSH sample from Vietri et al. (2018) (open triangles) are also reported. BAL AGNs are indicated with red circles.
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