Free Access

Fig. 6

image

Abundance of UDGs as a function of halo mass. Thick black points with errors: same as shown in Fig. 3, and these include the cluster points from vdB16. Black lines: best-fitting power-law relation including all black data points shown here. Blue squares: richnesses (i.e. the abundance of massive galaxies) in the same GAMA groups, with error bars defined in a similar way. Blue lines: best-fitting power-law relation to the richness points.

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.