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Fig. 10

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Number density of stars within a given mass bin as a function of stellar mass from the TF parameters (left) and from the MAP values (right). The red and blue lines show the distribution of the Clean and Uncertain sample groups, while the purple lines and purple-shaded areas indicate the distribution of all samples. We present the initial mass functions from Kroupa (2001) and Chabrier (2003) with pink and cyan lines, respectively.

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