Open Access

Fig. 8.


IRX–Zg relation for star-forming main sequence galaxies extracted at z = 1.5. The gas-phase metallicity is computed as the oxygen over hydrogen abundance Zg = 12 + log(O/H). We focus on the dense/fragmented gas-phase metallicity. The blue density shows the complete star-forming galaxy sample. The solid gray line shows the median trend of this sample. The dashed gray lines indicate the 15% and 85% quantiles of the distribution. We compare the G.A.S. model with observational measurements coming from Pannella et al. (2015) and Cortese et al. (2006).

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.