Fig. 6.
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Contribution of the young stellar models to the Ks luminosity function fit in the region dominated by hot dust emission in Sgr C (see Fig. 1). The solid line shows a Gaussian fit to the contribution of the 20 Myr model for Parsec (left panel) and MIST (right panel) models. The mean and the standard deviation of the Gaussian fits are indicated in each panel.
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