Free Access

Fig. 1.

image

Download original image

Distributions of SFRs (left) and of stellar masses (right) of source populations in our sample, subdivided into SFGs, RL, and RQ AGN. The distribution of SFRs of RL AGN extends to very low values, consistent with the fact that their radio emission is unrelated to the SFR; especially in the nearby universe they are generally associated with passive ellipticals. Both RQ and RL AGN preferentially reside in massive galaxies, with median stellar masses significantly higher than the mean stellar mass of SFGs. See text for more detailed comments.

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.