Fig. A.2.
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Observed 2D (upper panels) and 1D (lower panels) PRISM spectra of GHZ3. Symbols are the same as in Fig. 2. The Balmer (Lyman)-break feature is highlighted by the dashed vertical line, corresponding to z ∼ 1.76 (∼ 7.28). The lower redshift solution is compatible with the photometric redshift probability distribution P(z) discussed in Castellano et al. (2022).
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