The current status of the AKARI-FIS Point Source Catalogue is reported. The first version of the Bright Source Catalogue has been in public since March 2010 and used extensively in the various fields in astronomy. The second version of the Bright Source Catalogue and the first version of the Faint Source Catalogue are currently under development. The revised Bright Source Catalogue is expected to have improved completeness, reliability, and accuracy compared to the current version. The Faint Source Catalogue will have a scan-density dependent detection limit and will enable much deeper exploration of the sky especially in the high-ecliptic latitude regions. Both catalogues will be available in a year time scale.

ABSTRACT
1. INTRODUCTION
2. DATA DISTRIBUTION AND USAGE STATIS TICS
3. FUTURE PRODUCTS
    3.1. The Bright Source Catalogue Version 2
    3.2. The Faint Source Catalogue Version 1
4. DATA ARCHIVE ACTIVITY
    [Scan coverage data]
    [Event flux]
    [Rejected source catalogue]
5. SUMMARY
REFERENCES

• ISSEI YAMAMURA(Institute of Space and Astronautical Science, JAXA)
• SIN'ITIROU MAKIUTI(Institute of Space and Astronautical Science, JAXA)
• NORIO IKEDA(Institute of Space and Astronautical Science, JAXA)
• TATSUYA KOGA(Institute of Space and Astronautical Science, JAXA)
• AKIRA YOSHINO(Institute of Space and Astronautical Science, JAXA)
• CHISATO YAMAUCHI(Naitional Astronomical Observatory, NINS)