Free Access

Fig. 5.


Smoothed stellar population properties of quiescent galaxies for EMILES SSP models and Padova00 isochrones at 0.3 ≤ z <  0.5 as a function of their positions in the stellar mass–size plane (coloured dots, see colour bar in each panel). Top panels, from left to right: mass-weighted formation epoch, age, and metallicity, and bottom panels: extinction, luminosity surface brightness in the I band, and Sérsic index, respectively. To guide the eye, we illustrate the curve of constant formation epoch (black solid line) and its uncertainty (shaded area), as well as the stellar mass–size relation at this redshift bin (dotted black line).

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.