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Fig. 13
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Bins used to fit the MF between 0.3 and 0.7 M⊙ to the stars of the SC in the initial timestep (T = 0) of the main model. The fitted MF is shown with a solid line, and the MF determined using the MLE (with k fitted to best fit the bins) with a dashed line. The error bars show the Poisson uncertainties.
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