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Fig. 3.
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Flux density distribution of detected sources in ALMA Bands 6 and 7 in the A3COSMOS database versions 20180102 and 20220606 (including A3GOODSS). Flux densities are normalised to 1100 μm assuming that they probe the Rayleigh–Jeans tail of the dust continuum, with a dust spectral index β = 1.8 (Scoville et al. 2014).
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