Fig. D.1
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Same as Fig. 4 but for NGC 2419. For the King profile fitting, we used density values up to the background level, corresponding to ≈9′ from the cluster center. This is motivated by the fact that density values below the background level exhibit high signal-to-noise ratios, causing the MCMC algorithm to misinterpret and include them in the fit, leading to an inadequate result.
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