Fig. 4.
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Comparison of our z > 3 JWST-based rest-optical size–mass relations with z < 3 HST-based star-forming relations from Nedkova et al. (2021) and Mowla et al. (2019). The shaded regions indicate the 1σ fit uncertainties, while the intrinsic scatter is omitted for clarity. The slope of the 6 ≤ z < 9 relation is fixed (see Section 3.4).
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