Fig. 3.

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Example of random stamps of CEERS galaxies observed with the F200W filter, classified into four main morphological classes. Each panel of 16 images illustrates a different class. Top-left: spheroids. Top-right: disks. Bottom-left: irregulars. Bottom-right: composite bulge+disk galaxies. In each group of 16, galaxies are ordered by increasing photometric redshift (top to bottom) and stellar mass (left to right). The physical scale in kpc in shown for every galaxy. A square root scaling has been applied to enhance the outskirts.
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