IRX–AFUV relation derived from a sample of star-forming galaxies extracted at z = 1.5. The gray solid line indicates our best fit. For comparison we also plot the Buat et al. (2005) best fit (black solid line). Colored points show a subsample that is uniformly selected in the IRX–AFUV plan. The color scale shows the luminosity-weighted age of the stellar population hosted by the galaxy.
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.