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Fig. 8.


Comparison between the continuum luminosity at 5100 Å derived from the best-fit continuum power-law model with the luminosity of the broad Hα emission line, both in logarithmic scale, for the SUPER sample (blue circles). Both continuum and emission line luminosities are corrected for extinction (see Sect. 4.2). The SDSS sample from Shen & Liu (2012) and the sample from Mejía-Restrepo et al. (2016) are also shown (red and green circles, respectively). The best-fit linear relation (BCES Y|X regression) for the SUPER data is shown as a grey solid line.

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