Fig. C.2.
Download original image
Top panel: Stacked spectrum of 20 randomly selected AGN host galaxies, as confirmed by Comerford et al. (2024). This reveals a broad Hα component that is likely linked with outflows, which might be causing the observed kinematic gaseous asymmetries. Middle panel: Stacked spectrum of quenched galaxies showing no visible broad component. Bottom panel: Perfect single Gaussian fitting for emission lines without any potential outflow contribution.
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.