Fig. A.1.
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NIRSpec PRISM spectra of additional BB + emission line candidates at z ∼ 7 − 9, showing objects with clear or plausible Balmer breaks. Binned and unbinned spectra are shown for illustration. For comparison, we also over-plot the spectrum of the mini-quenched z = 7.3 galaxy from Looser et al. (2024), redshifted and rescaled to approximately match the observed flux blueward of the BB.
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