Fig. 5.
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Estimates, from left to right, of the total stellar mass formed, the SFR, and its first and second time derivatives, reconstructed at the present time (
) for the Gaussian synthetic SFHs with different ages and FWHMs, compared with the correct values (black contours). N increases from top to bottom, where the last row (SFR+) corresponds to the best positive-SFR polynomial fit.
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