Fig. 1.
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Source breakdown as a function of redshift for objects in our final catalog based on the cuts detailed in Section 3.1. Sources from different methods are shown in different panels: wide field spectroscopic surveys (top left), targeted spectra (top right), and HST Hyperion (bottom left). Rather than including a histogram of photometric redshift counts, we include the photometric redshift fraction (i.e. the fraction of galaxies with only a photometric redshift measured) for reference on the bottom right. The location of Hyperion is included in each panel as a shaded gray region (2.4 < z < 2.7), and insets for this shaded region are included for the spectroscopic and grism redshift panels. Histograms with multiple survey sources are stacked.
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