Recovering star formation histories: Integrated-light analyses vs. stellar colour–magnitude diagrams

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Fig. 7

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Same as Fig. 6, but using as spectral templates a set of 35 spectra generated from a constant SFR (t) and single metallicity (see text for details). However, in this case we do not use SSPs as spectral templates, and so we use a similar representation to the one used with STECKMAP (see Fig. 4).

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