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RADIO IDENTIFICATIONS IN THE NEP DEEP FIELD

  • White, Glenn J. (RAL Space, The Rutherford Appleton Laboratory) ;
  • Soto, Laia Barrufet de (RAL Space, The Rutherford Appleton Laboratory) ;
  • Pearson, Chris (RAL Space, The Rutherford Appleton Laboratory) ;
  • Serjeant, Stephen (Dept of Physical sciences, The Open University) ;
  • Lim, Tanya (RAL Space, The Rutherford Appleton Laboratory) ;
  • Matsuhara, Hideo (Inst of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Sirothia, S.K. (National Centre for Radio Astrophysics/TIFR, Pune University Campus) ;
  • Pal, S. (Indian Centre for Space Physics) ;
  • Karouzos, Marios (CEOU-Astronomy Program, Department of Physics & Astronomy, Seoul National University) ;
  • AKARI-NEP Team (Inst of Space and Astronautical Science, Japan Aerospace Exploration Agency)
  • Received : 2015.07.22
  • Accepted : 2016.10.25
  • Published : 2017.03.31

Abstract

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 r' magnitude brighter of 22.5 (to a completeness limit of 25.4 mag), and an average redshift ~ 0.8.

Keywords

References

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