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Fig. 5

image

From top to bottom panel: euclidean-normalized differential number counts of extragalactic sources at 250μm, 350μm, and 500μm, from the Herschel SPIRE Hermes survey by Oliver et al. (2010). Green datapoints come from the P(D) fluctuation analysis by Glenn et al. (2010). Lines are as in the previous figures.

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