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Fig. 14.


Outflow mass rate as a function of the logarithm of the bolometric luminosity for the BLR winds in the SUPER sample. Values from the WISSH sample (Vietri et al. 2018) (triangles) are also reported. BAL AGNs are denoted with red circles. The blue dashed line is the best-fit correlation of the CIV winds (SUPER+WISSH samples). Mass outflow rates of NLR winds from the SUPER sample are also reported (gold shaded area). The green shaded area shows the range probed by the outflow ionised phase in the NLR as found by Fiore et al. (2017), after rescaling the relation with the same assumption as for the Type-1 SUPER targets (see Kakkad et al. 2020 for further details). The dot-dashed line shows the log linear best-fit correlation of the X-ray winds.

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