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Fig. 2. | Earth, Planets and Space

Fig. 2.

From: Clustering of far-infrared galaxies in the AKARI All-Sky Survey North

Fig. 2.

Renormalized histograms of S90 fluxes of the AKARI FIS sources from the northern hemisphere: the solid line corresponds to the sample of identified galaxies with known redshifts, while the dashed line corresponds to the sources identified as galaxies but whose redshift is not known from the literature. Numbers on the left vertical axis correspond to the sample with known redshifts, while numbers on the right vertical axis correspond to the sample without known redshifts.

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