Free Access

Fig. 4.


Individual values of stellar population parameters of quiescent galaxies as a function of their size and median circularised radius (rc and , respectively) at 0.3 ≤ z <  0.5. From top to bottom: mass-weighted age, formation epoch, metallicity, and extinction for EMILES+Padova00 models. Each panel comprises a different stellar mass range. Vertical bars enclose the 1σ uncertainty level of individual values. Solid lines show the linear least-squares fitting to the distribution of values in each panel (see Eq. (2)), whereas the shaded region is its 1σ level uncertainty. Coloured markers illustrate the smoothed values obtained with the LOESS method (see Fig. 1).

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.