Fig. A.2.
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We show, as a function of redshift, the fraction of galaxies within Hyperion across all 100 MC iterations with redshifts determined from photometry (blue), ground-based spectroscopy (orange), and HST-grism spectroscopy (green). The lower-redshift portion of Hyperion is dominated by spectroscopic redshifts, whereas the higher-redshift portion is dominated by photometric redshifts.
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