Fig. 14
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Differential number counts at 220 and 280 GHz for dusty sources excluding IRAS counterparts, thus removing nearby luminous infrared galaxies. Consequently, the population consists mainly of high redshift lensed galaxies. At 220 GHz we include Everett et al. (2020) “dusty - zcut” counts, which also exclude IRAS sources. We note that the IRAS cut is more aggressive than just removing nearby sources, as almost all nearby sources are in IRAS.
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