천문학논총 (Publications of The Korean Astronomical Society)

  • 제27권4호
  • /
  • Pages.123-128
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  • 2012
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  • 1225-1534(pISSN)
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  • 2287-6936(eISSN)
한국천문학회 (The Korean Astronomical Society)
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OVERVIEW OF THE NORTH ECLIPTIC POLE DEEP MULTI-WAVELENGTH SURVEY (NEP-DEEP)

  • Matsuhara, H. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Wada, T. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Takagi, T. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Nakagawa, T. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Murata, K. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Churei, S. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency) ;
  • Goto, T. (Institute for Astronomy, University of Hawaii) ;
  • Oyabu, S. (Graduate School of Science, Nagoya University) ;
  • Takeuchi, T.T. (Graduate School of Science, Nagoya University) ;
  • Ohyama, Y. (Academia Sinica, Institute of Astronomy and Astrophysics) ;
  • Miyaji, T. (Instituto de Astronomia, Universidad Nacional Autonoma de Mexico) ;
  • Krumpe, M. (European Southern Observatory) ;
  • Lee, H.M. (Department of Physics & Astronomy, FPRD, Seoul National University) ;
  • Im, M. (Department of Physics & Astronomy, FPRD, Seoul National University) ;
  • Serjeant, S. (The Open University) ;
  • Peason, C.P. (Rutherford Appleton Laboratory Oxon) ;
  • White, G. (The Open University) ;
  • Malkan, M.A. (University of California) ;
  • Hanami, H. (Iwate University) ;
  • Ishigaki, T. (Iwate University) ;
  • Burgarella, D. (LAM, OAMP, Universite Aix-Marseille, CNRS) ;
  • AKARI NEP Team, AKARI NEP Team (AKARI NEP Team)
  • 투고 : 2012.07.08
  • 심사 : 2012.08.18
  • 발행 : 2012.09.16
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초록

An overview of the North Ecliptic Pole (NEP) deep multi-wavelength survey covering from X-ray to radio wavelengths is presented. The main science objective of this multi-wavelength project is to unveil the star-formation and AGN activities obscured by dust in the violent epoch of the Universe (z=0.5-2), when the star formation and black-hole evolution activities were much stronger than the present. The NEP deep survey with AKARI/IRC consists of two survey projects: shallow wide (8.2 sq. deg, NEP-Wide) and the deep one (0.6 sq. deg, NEP-Deep). The NEP-Deep provides us with a $15{\mu}m$ or $18{\mu}m$ selected sample of several thousands of galaxies, the largest sample ever made at these wavelengths. A continuous filter coverage at mid-IR wavelengths (7, 9, 11, 15, 18, and $24{\mu}m$) is unique and vital to diagnose the contribution from starbursts and AGNs in the galaxies at the violent epoch. The recent updates of the ancillary data are also provided: optical/near-IR magnitudes (Subaru, CFHT), X-ray (Chandra), FUV/NUV (GALEX), radio (WSRT, GMRT), optical spectra (Keck/DEIMOS etc.), Subaru/FMOS, Herschel/SPIRE, and JCMT/SCUBA-2.

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참고문헌

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