Fig. 4
Expected variation of the flux density S(T) for a truncated star formation history in the FUV and NUV-bands and in the newly defined LyC (Hα), Hβ, Hγ, and Hδ pseudo-filters after a total quenching of the star formation activity (quenching factor QF = 1) with respect to that of an unperturbed galaxy (S(NT)) as a function of the quenching age QA for a model galaxy with properties given in Table 5.
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