Fig. 5.

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Density profiles. The solid circles show the radial density profile of Rup 106 (left panel) and IC 4499 (right panel) corrected for the contamination from the background and foreground stars. The open circles indicate the background and foreground uncorrected counts. The density of field stars was estimated using the most external bins. The best-fit King model is shown as a solid line on the figures while the small panel at the bottom of the figures shows the residual of the fit at each radial bin. The parameters of the best-fit King model are also indicated in the figure.
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