We have imaged the AKARI Deep Field with the GMRT radio telescope at 610 MHz, detecting 1224 radio components, which are optically identified with 455 optical galaxies having a mean r0 magnitude brighter of 22.5 (to a completeness limit of 25.4 mag), and an average redshift ~ 0.8.

ABSTRACT
1. INTRODUCTION
2. RADIO SURVEY
3. CROSS-IDENTIFICATIONS
4. CONCLUSIONS
REFERENCES

• Glenn J. White(RAL Space, The Rutherford Appleton Laboratory/Dept of Physical sciences, The Open University)
• Laia Barrufet de Soto(RAL Space, The Rutherford Appleton Laboratory)
• Chris Pearson(RAL Space, The Rutherford Appleton Laboratory/Dept of Physical sciences, The Open University)
• Stephen Serjeant(Dept of Physical sciences, The Open University)
• Tanya Lim(RAL Space, The Rutherford Appleton Laboratory)
• Hideo Matsuhara(Inst of Space and Astronautical Science, Japan Aerospace Exploration Agency)
• S.K.Sirothia(National Centre for Radio Astrophysics/TIFR, Pune University Campus)
• S.Pal(Indian Centre for Space Physics)
• Marios Karouzos(CEOU-Astronomy Program, Department of Physics & Astronomy, Seoul National University)
• AKARI-NEP Team(Inst of Space and Astronautical Science, Japan Aerospace Exploration Agency)