Fig. 4.
From: Clustering of far-infrared galaxies in the AKARI All-Sky Survey
Angular correlation function, in linear and logarithmic bins, in the northern (left panel) and southern (right panel) hemisphere of the AKARI All-Sky Survey. In both panels linear bins are marked by full triangles, connected by a solid line, while logarithmic bins are shown as full circles connected by a dashed line. Note the difference in scale of the panels.