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Fig. 5.

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Multi-wavelength analysis of CEERS-1019. The left panel shows cutout images around CEERS-1019 in the NIRCam filters. In the F150W sub-panel, we show the positions of the three compact clumps resolved only at short wavelength, labeled A, B, and C (blue, green, and red, respectively) The right panel shows the SED best-fit models using CIGALE (Boquien et al. 2019) of the integrated light of CEERS-1019 (“total” in black), as well as the individual clumps (A, B, and C in blue, green, and red, respectively). Observed fluxes are marked with circles, while the predicted fluxes from the best fit are marked with crosses.

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