We present the first measurement of the angular two-point correlation function for AKARI 90μm point sources, detected outside of the Milky Way plane and selected as candidates for extragalactic sources. This is the first measurement of the large-scale angular clustering of galaxies selected in the far-infrared after IRAS. We find a positive clustering signal in both hemispheres extending up to ~ 40 degrees, without any significant fluctuations at larger scales. The observed correlation function is well fitted by a power law function. However, southern galaxies seem to be more strongly clustered than northern ones and the difference is statistically significant. The reason for this difference - technical or physical - is still to be found.

ABSTRACT
1. INTRODUCTION
2. ANGULAR CLUSTERING OF AKARI ALL-SKY SURVEY GALAXIES
REFERENCES

• A. POLLO(Astronomical Observatory of the Jagiellonian University, National Centre for Nuclear Research, Centre for Theoretical Physics of the Polish Academy of Sciences)
• T. T. TAKEUCHI(Division of Particle and Astroph. Science, Nagoya University)
• T. L. SUZUKI(Division of Particle and Astroph. Science, Nagoya University)
• S. OYABU(Division of Particle and Astroph. Science, Nagoya University)