Fig. 5.From: Clustering of far-infrared galaxies in the AKARI All-Sky SurveyPower-law fit to the angular correlation function of extragalactic sources, measured in the northern (full circles, solid line) and southern (full triangles, dashed line) hemisphere of the AKARI All-Sky Survey. Points correspond to the measurements in the logarithmic bins, while lines show the best power-law fit.Back to article page