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Fig. 8.


Spectral energy distribution (SED) of QSO1 (blue) and QSO2 (orange), used as incident radiation in the Cloudy calculations. We compare the models with the available MUSE data (lighter color for each quasar). Left panel: the vertical lines indicate the energies used to define the different power-laws (Sect. 5.2.1). Right panel: zoomed in version of the box highlighted in the left panel. The emission from the wavelength ranges around the C IV and Lyα line locations are masked to prevent contributions from resonantly scattered photons, as done in Arrigoni Battaia et al. (2015b).

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