Fig. 1.
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Redshift distribution of the galaxies used in this study, which includes 125 out of the 137 sources from the z-GAL sample. In our analysis, we exclude multiples at different redshifts in the field of view observed by NOEMA, which are unresolved in the Herschel field of view, as well as problematic sources (see details in Sect. 2.2).
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