Free Access

Fig. 5

thumbnail

Probability density distributions of stellar masses (log   Ms, in log   M), (left panel) and probabilities of being late type (pl, right panel), for red, low SFR galaxies (red lines), blue, high SFR galaxies (blue lines), and for red, high SFR galaxies (grey lines) in the superclusters of filament (solid lines) and spider (dashed lines) morphology. High SFR galaxies have log   SFR ≥ −0.5, and low SFR galaxies have log   SFR < −0.5. Lines in the left panel denote the same populations as in the right panel.

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.