Free Access

Fig. A.1


Spectral energy distributions of two quasars with good visible/UV detections. Left panels: include a power-law component (dash-dotted pink) representing the emission from the hot accretion disk. Right panels: exclude that component, and show the components considered when fitting the quasars in this work. Other individual components as described in Fig. 2.

This figure is made of several images, please see below:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.