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The Korean Astronomical Society (한국천문학회)
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THE AGN POPULATION IN THE AKARI NEP DEEP FIELD

  • Soto, Laia Barrufet de (RAL Space, The Rutherford Appleton Laboratory) ;
  • White, Glenn J. (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) ;
  • Oi, Nagisa (Inst of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Karouzos, Marios (Astronomy Program, Department of Physics & Astronomy, Seoul National University) ;
  • AKARI-NEP Team (Inst of Space and Astronautical Science, Japan Aerospace Exploration Agency)
  • Received : 2015.07.21
  • Accepted : 2016.10.15
  • Published : 2017.03.31
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Abstract

The AKARI North Ecliptic Pole Deep Field is a natural location to accomplish deep extragalactic surveys. It is supported by comprehensive ancillary data extending from radio to X-ray wavelengths, which have been used to classify radio sources as radio-loud and radio-quiet objects and to create a catalogue of Active Galactic Nuclei (AGN). This has been achieved by using a radio-optical classification and colour-colour diagrams rather than the more usual way based on spectroscopy Furthermore, we explore whether this technique can be extended by using a far-Infrared (FIR) colour-colour diagram which has been used to identify 268 high redshift candidates.

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References

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