Updated CEERS catalog photometry errors vs. CEERS ASTRODEEP-JWST photometry errors for the sources in common between the two catalogs (displayed as gray dots) for a sample band (F356W). The bisector of the plot is represented as a dashed black line surrounded by a 1σ confidence interval (shaded black area) representing the typical dispersion of the data points around the bisector. A power-law fit is displayed to showcase how the updated CEERS catalog’s errors tend to be higher with respect to CEERS ASTRODEEP-JWST ones.