Fig. 4.
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CIGALE SED models derived from the single and mixed stellar population scenarios described in Sect. 4.2. Blue (orange) line and squares represent the SED models and the expected fluxes for NIRCam/MIRI filters derived using a single τ-decaying (mixed) stellar population. Black line and triangles represent the NIRSpec/Prism spectra and the NIRCam+MIRI photometry, respectively. The blue and orange lines have been convolved to match de NIRSpec/Prism resolution (R = 100).
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