Overview of North Ecliptic Pole Deep multi-wavelength Survey (NEP-Deep)
Abstract
The recent updates of the North Ecliptic Pole deep (0.5~deg, NEP-Deep) multi-wavelength survey covering from X-ray to radio-wave is presented. The NEP-Deep provides us with several thousands of 15~m or 18~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~m) is unique and vital to diagnose the contributions from starbursts and AGNs in the galaxies out to =2.The new goal of the project is to resolve the nature of the cosmic star formation history at the violent epoch (e.g. =1--2), and to find a clue to understand its decline from =1 to present universe by utilizing the unique power of the multi-wavelength survey. The progress in this context is briefly mentioned.
Cite
@article{arxiv.1710.10472,
title = {Overview of North Ecliptic Pole Deep multi-wavelength Survey (NEP-Deep)},
author = {H. Matsuhara and T. Wada and N. Oi and T. Takagi and T. Nakagawa and K. Murata and T. Goto and S. Oyabu and T. T. Takeuchi and K. Malek and A. Solarz and Y. Ohyama and T. Miyaji and M. Krumpe and H. M. Lee and M. Im and S. Serjeant and C. P. Pearson and G. J. White and M. A. Malkan and H. Hanami and T. Ishigaki and D. Burgarella and V. Buat and A. Pollo},
journal= {arXiv preprint arXiv:1710.10472},
year = {2017}
}
Comments
4 pages, 2 figures, AKARI conference proceedings; accepted to PKAS