Fig. 1.
Comparison of light-weighted, mean stellar population properties of NGC 1433, derived at a S/N of 40 (upper panels), 80 (centre panels), and 100 (lower panels). Each set of panels displays age, metallicity, and [α/Fe] enhancements. The limits of the colour bar are stated in the lower-right corner of each panel. Based on the reconstructed intensities from the MUSE cube, we display isophotes in steps of 0.5 mag. North is up; east is to the left.
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.