Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group

Open Access

Fig. 14.

Colour profiles for NGC 1549, NGC 1553, and NGC 1546. Left: I_E − J_E. Right: Y_E − H_E. Such plots allow for the analysis of the differences between the galaxy profiles. In particular, the profile of NGC 1549 is the flattest, while that of NGC 1546 is the steepest across all colours.

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.