Fig. 3.

Angular correlation function in the AKARI All-Sky Survey North— comparison of subsamples with different limits of flux density S90. Points correspond to the measurements in the logarithmic bins and lines show the best power-law fit. Full triangles and the solid line correspond to the whole sample, i.e. S₉₀ > 0.2 Jy. Full circles and the short-dashed line correspond to the sample with a limit S₉₀ > 0.5 Jy. Open circles and the dotted line correspond to the sample limited by S₉₀ > 1 Jy. The brightest sample, S₉₀ > 1.5 Jy, is shown by open squares and the long-dashed line.