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Fig. D.1.
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MEH and SFH median curves and 16th-84th percentiles resulting from the fits of two galaxies with Δτ ≤ 1 Gyr (left) and Δτ > 1 Gyr (right), whose best-fit spectra have been fitted 100 times after the reshuffle of the residuals and Gaussianly adding them to it.
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