Left: [F444W] magnitude vs. [F356W]−[F444W] colour of the F200W-dropout sample in the four NIRCam pointings (coloured points and histograms, named N1, N2, N3, and N6) and for full CEERS sample (black dots and grey histogram). Points with a red edge are objects in the F200W-dropout-extra sub-sample. Empty symbols indicates objects in our sample with a S/N < 3 in the F356W filter and we assigned, for visual purposes, a colour of [F356W]−[F444W] = 4 to galaxies with redder colours. We also report the sample of F200W-dropouts by Rodighiero et al. (2023, green empty stars), highlighting their two candidates at z > 10, namely KABERLABA and PENNAR, and the sample by Yan et al. (2023a, brown empty pentagons). Right: normalised [F356W]−[F444W] colour density distribution. Each histogram is normalised so that its integral is equal to one.