Fig. 20

SFR vs. stellar mass of cluster galaxies. Individual values are those computed by Annunziatella et al. (2014) and are shown here for different spectral classes. Black solid circles and small squares indicate biweight means with bootstrap errors for vsELGs and mELGs+sELGs considering three bins per order of magnitude in stellar mass.
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.