Fig. 1.
From: Clustering of far-infrared galaxies in the AKARI All-Sky Survey North
Renormalized histograms of redshifts z of two samples of the AKARI FIS sources from the northern hemisphere. The solid line corresponds to the “full” sample with S90 ≥ 0.2 Jy, while the dashed line corresponds to the sources from the brightest sample with S90 ≥ 1.5 Jy. Numbers on the left vertical axis correspond to the S90 ≥ 0.2 Jy case, while numbers on the right vertical axis correspond to the S90 ≥ 1.5 Jy sample.