Free Access

Fig. 4.


Number of detectable DWDs in the log satellite mass – log distance parameter space for different SFH models: exponentially decreasing, constantly star-forming at the rate of 1 M yr−1 and single burst 13.5 Gyr ago. White stars represent known satellites listed in Table 2. The top x-axes shows the absolute magnitude in the V−band. The bottom panel is cut at log d∼1.6 as there are no more detectable sources at larger distances; this is the case of ultra-faint dwarfs, which have no sources detectable beyond this distance.

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.