Fig. 11
Stellar population parameters of the young population for the ELG sample, obtained from the SED fitting. Top left panel: distribution of age of the young stellar population, in millions of years. Top right panel: distribution of metallicity of the young stellar population, both as a fraction of heavy elements Z and as oxygen abundance 12 + log(O/H). Bottom left panel: distribution of extinction of the young stellar population, in AV magnitudes.Bottom right panel: distribution of stellar mass of both young and old stellar populations (SP), in blue and red, respectively.
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