Fig. 17.

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Examples of photometric redshift fits made with EAZY for ≳8 galaxies in MIDIS. The insets show: (i) the source identification and redshift estimates; and (ii) F560W 2″ × 2″ thumbnails. The second (from top) panel on the right shows a source for which the addition of MIRI changed the photometric redshift solution from z = 2.9 to 10.7 due to the bright F560W flux being identified with Hβ + [O III].
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