Line equivalent width for the spectral lines in [OII] as a function of the stellar mass range (left panel) and of the local density range (right panel) for the stacked spectra. We apply no dust correction to the stacked derived values since we assume spatial coincidence between the continuum and line-emitting regions, and they are affected by dust in a similar manner.
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.