We have identified 22 quasars in the AKARI far-infrared all-sky Bright Source Catalogue, using a matching radius of < 10", and excluding matches which are close to foreground extended sources or cirrus. We have confirmed a relation between quasar optical luminosity and far-infrared luminosity which was found in an earlier study. In addition, we have found that the 11 sources which are at redshift z > 1 are magnified with respect to the predicted far-infrared luminosity, and consider this may be due to gravitational lensing. If confirmed, this would provide a new way to identify lenses; if not, we may have identied an interesting new population of extreme starbursting quasars.

ABSTRACT
1. INTRODUCTION
2. QUASAR CATALOGUES
3. METHODS AND RESULTS
REFERENCES

• Chris Sedgwick(The Open University)
• Stephen Serjeant(The Open University)
• Chris Pearson(RAL Space, Rutherford Appleton Laboratory/The Open University)
• I. Yamamura(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• S. Makiuti(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• N. Ikeda(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• Y. Fukuda(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• S. Oyabu(Graduate School of Science, Nagoya University)
• T. Koga(Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• S. Amber(The Open University)
• Glenn J. White(The Open University/RAL Space, Rutherford Appleton Laboratory)