Fig. 8
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Examples of incident spectra constructed using SED fitting parameters from the L16 catalogue and empirical and theoretical relations for the emission lines. Top: spectra of galaxies with different stellar mass, indicated on the figure in log10(M* [M⊙]), and at z = 0.9. Bottom: spectra of galaxies at different redshift and with stellar mass equal to 9.5 in log10(M* [M⊙]).
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