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Fig. 2

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Two-dimensional representation of one low-mass and one high-mass cluster generated with DMCMC and EMCMC, respectively. For comparison, the corresponding projections are illustrated also for the hydrodynamically simulated clusters m1.e4 and m9.e4 from the work of Ballone et al. (2020). The x and y coordinates are measured in parsecs. For EMCMC, we show the value of the hyper-parameter J (maxJump) and the total mass expressed in M103=1000$\[M_{10^3 \odot}=1000\]$ solar masses.

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