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Fig. 8.

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K-band magnitude distribution of detected sources in the Trumpler 14 cluster with the CHIPS (orange; K1) and MAD (blue;KS) samples as a function of angular separation from the central star. Sources within 01 from one another are connected by a solid red line. MAD sources brighter than K = 8 are likely impacted by non-linearity and/or saturation effects impacting the MAD observations.

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