Free Access

This article has an erratum: [erratum]

Fig. A.5

image

Difference between output from fado for spectral fits with the Base and input value of stellar mass a), mean light- and mass-weighted stellar age b) and c), mean light- and mass-weighted stellar metallicity d) and e), and mean percentual deviation of the Hα emission-line equivalent width f). The synthetic input spectra were computed with Rebetiko assuming an instantaneous burst star formation scenario. In panel f) the blue points correspond to equivalent-width of Hα in emission below 0.5 Å and the magenta points mark values in the range 0.5 Å ≤ EW(Hα) ≤ 1 Å. The green lines are three times the standard deviation over the whole age range of the models. The vertical blue strips on top of the diagrams depict the ages of the SSPs composing Base .

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.