Fig. 9.
Fraction of Lum[OIII] > 106.4 L⊙ as a function of stellar mass, log(M*), for barred AGN galaxies (solid lines) and AGNs in pairs with restrictions in the galaxy pair companion properties defined in the text (dotted and dot-dashed lines). The gray surfaces represent the control sample within uncertainties derived through the bootstrap resampling technique. Each bin for each sample contains a similar number of galaxies. The average number of galaxies in each bin is ≈105 for barred-agn, ≈140 for CS and ≈67 for agn in pairs with restrictions in the properties of the galaxy pair companion.
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.