Fig. 10.
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Upper panel: Evolution of the UV simulation sizes (y-axis, in kpc) as function of stellar mass (x-axis) for z ∈ [5, 10]. Lower panel: Evolution of sizes from mock observations as function of stellar mass. Size mass relation for simulated observations from Costantin et al. (2023) and LaChance et al. (2024) and NIRCAM observations from Ward et al. (2024). CEERS data has been taken from Morishita et al. (2024) and Ormerod et al. (2024).
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