Fig. 2
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Predicted spectrum of GS-z14-0 based on the SFH of the galaxy shown in Fig. 1, and for an ionization parameter U = −1.2. The spectrum has been computed using BAGPIPES (Carnall et al. 2018). It has a UV spectral slope β = −2.25; the position of the CIII]λ1907, 1909 line is indicated, along with those potentially detected by MIRI (Helton et al. 2024).
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