Fig. B.1.
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Example of random stamps of the same galaxies in CEERS (F150W) and CANDELS (F160W) at the same pixel scale with different morphological classifications. Two top panels show galaxies classified as late-type in CEERS (top-left) and as early-type in CANDELS (top-right). The bottom panels show galaxies classifed as disks in CEERS (botttom-left) and irregular in CANDELS (bottom-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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