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Fig. 5


The cumulative fractions of galaxies of different SED classes as a function of LIR, for the z ∪ zp sample. The pink, blue, green, and black-shaded regions correspond to the fractions of SBGs, PSBGs, SFGs, and ETGs, respectively (as labeled). The orange and red-shaded regions correspond to the fractions of SED-identified AGNs (mostly at low LIR) and AGNs identified in Paper 2 from X-ray or radio emission, respectively.

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