Deep Extragalactic Surveys around the Ecliptic Poles with AKARI (ASTRO-F)

@article{Matsuhara2006DeepES,
  title={Deep Extragalactic Surveys around the Ecliptic Poles with AKARI (ASTRO-F)},
  author={Hideo Matsuhara and Takehiko Wada and Shuji Matsuura and Takao Nakagawa and Mitsunobu Kawada and Youichi Oyama and Chris Pearson and Shinki Oyabu and Toshinobu Takagi and Stephen Serjeant and Glenn J. White and Hitoshi Hanami and Hidenori Watarai and Tsutomu T. Takeuchi and Tadayuki Kodama and Nobuo Arimoto and Sadanori Okamura and Hyung-Mok Lee and Soojong Pak and Myungshin Im and Myung Gyoon Lee and Woojung Kim and Woong-Seob Jeong and Koji Imai and Naofumi Fujishiro and Mai Shirahata and Toyoaki Suzuki and Chiaki Ihara and Itsuki Sakon},
  journal={Publications of the Astronomical Society of Japan},
  year={2006},
  volume={58},
  pages={673-694}
}
AKARI (formerly ASTRO-F) is an infrared space telescope designed for an all-sky survey at 10-180 µm, and deep pointed surveys of selected areas at 2-180 µm. The deep pointed surveys with AKARI will significantly advance our understanding of galaxy evolution, the structure formation of the Universe, the nature of the buried AGNs, and the cosmic infrared background. Here we describe the important characteristics of the AKARI mission: the orbit, and the attitude control system, and investigate the… 
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Aims. The Westerbork Radio Synthesis Telescope, WSRT, has been used to make a deep radio survey of an ∼1.7 degree 2 field coinciding with the AKARI north ecliptic pole deep field. The observations,
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We have carried out a survey of the north and south ecliptic poles, EP-N and EP-S, respectively, with the Spitzer Space Telescope and the Wide-field Infrared Survey Explorer (WISE). The primary
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ASTRO-F is the Japanese infrared astronomical satellite. The mission purpose is the infrared sky survey with much higher sensitivities and spatial resolutions than those of the previous survey
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