Free Access
Fig. 3
Observed uncertainties of the MZ relations for star-forming and passive galaxies by Peng et al. (2015) are reported with blue lines. We show with orange lines the third-order polynomial fits for the passive and star-forming galaxies adopted in this article.
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.