Fig. A.1
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Markov chain Monte Carlo chains for open clusters IC4665, NGC6005, and NGC2243. The first row shows the raw chain and the second row shows the converged part of the chain. Plots from left to right are posterior, positions for the IMF αIMF, rate of SNIa log10(NIa), star formation efficiency log10(S F E), and the peak and shape of star formation log10(S F Rpeak). The cyan line shows the prior value and the red line shows the best-fit value.
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