Fig. 15.
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Redshift distribution predicted in SPRITZ for galaxies with [N III]57 μm, [O III]52 μm, and/or [O III]88 μm lines above 10−19 W/m2. The hatched histogram shows the subpopulation that is also detected in the Deep and Wide PRIMAger surveys, considering the conservative depths. The grey area shows the redshift range in which [N III]57 μm and [O III]52 μm lines are in the PRIMA/FIRESS wavelength coverage.
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