Top: percentage of [NeV] emitters as a function of stellar mass for the green, red and blue galaxies. The fraction of the [NeV] emitters increases with mass in the blue cloud and decreases in the red sequence, but no statistical trend is observed in the green valley. Bottom: luminosities in the [NeV] line as a function of stellar mass. Symbols as in Fig. 4. Solid, dashed, and dotted lines show the least squares fits to the blue, green, and red [NeV] emitters, respectively. An increasing [NeV]λ3426 line luminosity is observed at larger stellar masses.
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.