It is a long known fact that there exists a tight correlation between far-infrared and radio emission both for galaxies hosting active galactic nuclei and for star forming galaxies. We probe the radio - infrared correlation for a sample of extragalactic sources constructed by the cross-correlation of the AKARI/IRC All-Sky Survey Point Source Catalogue, the AKARI/FIS All-Sky Survey Bright Source Catalogue, and the NRAO VLA Sky Survey. Additionally, all objects of our sample were identified as galaxies in NED and SIMBAD databases, and a part of them is known to host active galactic nuclei (AGNs). After remeasuring all the fluxes, in order to avoid small aperture effects, we compare the ratio of radio to infrared emission from different types of extragalactic sources, and discuss the FIR/radio correlation as seen by AKARI and make a comparison to the previous results obtained thanks to IRAS.

ABSTRACT
1. INTRODUCTION
2. SAMPLE SELECTION
3. PRELIMINARY RESULTS
4. SUMMARY
REFERENCES

• A. PEPIAK(Astronomical Observatory of the Jagiellonian University)
• A. SOLARZ(Department of Particle and Astrophysical Science, Nagoya University)
• A. POLLO(Astronomical Observatory of the Jagiellonian University, National Centre for Nuclear Research)
• T. T. TAKEUCHI(Department of Particle and Astrophysical Science, Nagoya University)
• W. JURUSIK(Astronomical Observatory of the Jagiellonian University)
• AKARI TEAM