Mass and dust extinction A_V from z = 0 to 7 for the F200W-dropout sample (colored points) and the entire CEERS sample in NIRCam2 (black dots). We also report the median A_V at different stellar masses for the general CEERS sample with good SED fit (red squares), when at least ten galaxies are present in the stellar mass bin. We also report the expected relation derived assuming a Calzetti et al. (2000)’s reddening law and an intrinsic UV slope of −2.3 (green dotted lines; McLure et al. 2018).