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Fig. 11.

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Top panels: best-fit SEDs of CIGALE at different redshifts, marked on top of each column. Coloured horizontal bars indicate the MIRI filters planned for the CEERS survey. Boxes on the left of each panel show the percentage of detection at a given filter. Galaxies are classified according to the SFR with the starting sample on the top row, the ‘low’ subsample in the middle, and the ‘high’ subsample on the bottom row. Median values of each sample are reported in the bottom right of the first panel in each row and Table 5. Bottom panel: same analysis selecting galaxies according to their stellar masses, as reported in Table 5.

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