Fig. 13

Central region of the Abell 2457 galaxy cluster (26.5 × 18.2 arcmin) analyzed using our dust identification pipeline (see text for details). Upper panel: sum of the g, r and i bands with a color scale tuned to obtain an optimal contrast between sources of different surface brightness. Bottom panel: same region as the upper panel showing those pixels compatible with dust (yellow pixels) according with our analysis.
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.