Fig. 10
Observed UV to FIR SED of NGC 4569 (HRS 217) (red filled dots) is compared to the best-fit model derived by CIGALE using a truncated star formation history (black solid line) or a normal delayed star formation history (blue dotted line) (upper panel). The normalised difference between the observed and model value in the different photometric bands is plotted vs. lambda in the lower panel (for a truncated star formation history).
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