Overview of North Ecliptic Pole Deep multi-wavelength Survey (NEP-Deep)

Autor: Matsuhara, H., Wada, T., Oi, N., Takagi, T., Nakagawa, T., Murata, K., Goto, T., Oyabu, S., Takeuchi, T.T., Malek, K., Solarz, A., Ohyama, Y., Miyaji, T., Krumpe, M., Lee, H.M., Im, M., Serjeant, S., Pearson, C.P., White, G.J., Malkan, M.A., Hanami, H., Ishigaki, T., Burgarella, D., Buat, V., Pollo, A.
Přispěvatelé: Laboratoire d'Astrophysique de Marseille (LAM), Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Rok vydání: 2017
Předmět:
Zdroj: Matsuhara, H; Wada, T; Oi, N; Takagi, T; Nakagawa, T; Murata, K; et al.(2018). Overview of North Ecliptic Pole Deep multi-wavelength Survey (NEP-Deep). 2017, Publications of The Korean Astronomical Society, vol. 32, issue 1, pp. 213-217. UCLA: Retrieved from: http://www.escholarship.org/uc/item/01t815th
Publications of The Korean Astronomical Society
Publications of The Korean Astronomical Society, 2017, 32 (1), pp.213-217. ⟨10.5303/PKAS.2017.32.1.213⟩
ISSN: 2287-6936
1225-1534
DOI: 10.5303/PKAS.2017.32.1.213⟩
Popis: The recent updates of the North Ecliptic Pole deep (0.5~deg$^2$, NEP-Deep) multi-wavelength survey covering from X-ray to radio-wave is presented. The NEP-Deep provides us with several thousands of 15~$\mu$m or 18~$\mu$m selected sample of galaxies, which is the largest sample ever made at this wavelengths. A continuous filter coverage in the mid-infrared wavelength (7, 9, 11, 15, 18, and 24~$\mu$m) is unique and vital to diagnose the contributions from starbursts and AGNs in the galaxies out to $z$=2.The new goal of the project is to resolve the nature of the cosmic star formation history at the violent epoch (e.g. $z$=1--2), and to find a clue to understand its decline from $z$=1 to present universe by utilizing the unique power of the multi-wavelength survey. The progress in this context is briefly mentioned.
Comment: 4 pages, 2 figures, AKARI conference proceedings; accepted to PKAS
Databáze: OpenAIRE
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