Fig. A.2.
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Comparison or morphological fractions of early vs. late (top panel) and Hubble types vs. peculiar (bottom panel) between CEERS Huertas-Company et al. 2024 (dotted lines) and COSMOS-Web (solid lines). The optical rest-frame morphologies are plotted. At z < 1 we use F150W; at 1 < z < 3 we use F356W for CEERS and F277W for COSMOS-Web; and at z > 3 we use F444W.
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