Fig. 5
The input and recovered SFHs of a series of short (10 Myr) bursts of star formation at different input age. The black, solid histogram shows the input SFH, given the binning adopted. The red histograms show the recovered SFH, along with the fit of a Gaussian distribution as the dashed line. The mean (μ) and variance (σ) of the fitted Gaussian distribution are also listed.
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