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Overview of the North Ecliptic Pole multi-wavelength survey (NEP-DEEP)

Matsuhara, H.; Wada, T.; Takagi, T.; Nakagawa, T.; Murata, K.; Churei, S.; Goto, T.; Oyabu, S.; Takeuchi, T. T.; Ohyama, Y.; Miyaji, T.; Krumpe, M.; Lee, H. M.; Im, M.; Serjeant, S.; Peason, C. P.; White, G.; Malkan, M. A.; Hanami, H.; Ishigaki, T.; Burgarella, D. and AKARI NEP Team, AKARI NEP Team (2012). Overview of the North Ecliptic Pole multi-wavelength survey (NEP-DEEP). Publications of The Korean Astronomical Society, 27(4) pp. 123–128.

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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 star-formation and black hole activities were much stronger than at 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 μm or 18 μm 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 μm) 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.

Item Type: Journal Item
Copyright Holders: 2012 The Korean Astronomical Society
ISSN: 2287-6936
Keywords: infrared; galaxies; starburst; AGN; dust
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Research Group: Space
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Item ID: 36486
Depositing User: G. J. White
Date Deposited: 04 Feb 2013 10:47
Last Modified: 07 Dec 2018 10:13
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