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

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.; Pearson, C.P; Serjeant, Stephen; White, G. J.; Malkan, M.A.; Hanami, H.; Ishigaki, T.; Burgarella, D.; Buat, V. and Pollo, A. (2017). Overview of North Ecliptic Pole deep multi-wavelength survey (NEP-DEEP). Publications of The Korean Astronomical Society, 32(1) pp. 213–217.

DOI: https://doi.org/10.5303/PKAS.2017.32.1.213

Abstract

The recent updates of the North Ecliptic Pole deep (0.5 deg2 , NEP-Deep) multi-wavelength survey covering from X-ray to radio-wave is presented. The NEP-Deep provides us with several thousands of 15 µm or 18 µm selected galaxies, which is the largest sample ever made at these wavelengths. A continuous filter coverage in the mid-infrared wavelength (7, 9, 11, 15, 18, and 24 µm) 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 multiwavelength survey. The progress in this context is briefly mentioned.

Viewing alternatives

Look up in Google Scholar

Metrics

Public Attention

Altmetrics from Altmetric

Number of Citations

Citations from Dimensions

Item Actions

Export

About

CORE (COnnecting REpositories)

Recommendations