Figure 5.
Edge-on view of the stars born in a KCD at $z \sim 7.2$ (top-left panel) and of those born in another KCD at $z \sim ~4.9$ (bottom-left panel), alongside the same stars at the concluding snapshot of the simulation, at $z = 4.4$ (right-hand panels). We employed 150 bins in both axes, covering a range from −1.2 to 1.2 kpc. Only bins containing a minimum of 50 particles are displayed, highlighting the trend while minimizing noise of the outliers.

Edge-on view of the stars born in a KCD at |$z \sim 7.2$| (top-left panel) and of those born in another KCD at |$z \sim ~4.9$| (bottom-left panel), alongside the same stars at the concluding snapshot of the simulation, at |$z = 4.4$| (right-hand panels). We employed 150 bins in both axes, covering a range from −1.2 to 1.2 kpc. Only bins containing a minimum of 50 particles are displayed, highlighting the trend while minimizing noise of the outliers.

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