Fig. 2
High-resolution three-color WISE images (W1 in blue, W2 in green, W3 in red) of NGC 1316 (left panel) and NGC 612 (right panel). The dust lanes are clearly seen. The super-resolution technique creates artifact features around high surface brightness emitters (e.g. nuclei, stars; see Sect. 3 for further details). 1 arcmin corresponds to 5.8 kpc in NGC 1316 and to 36.6 kpc in NGC 612.
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.