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Fig. 13.

image

Top: [OIII] EW in logarithm as a function of the velocity shift of the CIV emission line for the SUPER sample (diamonds), colour-coded according to the EW[OIII]. Additionally, the WISSH sample with reliable [OIII] measurements is also reported (empty triangles). Bottom: velocity of [OIII] at 10% of the line flux as a function of the velocity shift of the CIV emission line for the SUPER sample (blue diamonds). The WISSH subsample with reliable [OIII] measurements is also shown as green triangles. BAL AGNs are indicated with red circles.

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