WISH: Wide-field imaging surveyor for high-redshift

Toru Yamada, Mamoru Doi, Tomotsugu Gotc, Yuji Ikeda, Masatoshi Imanishi, Akio Inoue, Satoru Iwamura, Ikuru Iwata, Nobuyuki Kawai, Masakazu A.R. Kobayashie, Tadayuki Kodama, Yutaka Komiyama, Hideo Matsuhara, Yoshiki Matsuoka, Tomoki Morokuma, Kouji Ohta, Shinki Oyabu, Yoichi Sato, Hiroyuki Sugita, Ryo TsutsuiChihiro Tokoku, Saku Tsuneta, Takehiko Wada, Kiyoto Yabe, Naoki Yasuda, Daisuke Yonetoku

研究成果: Conference contribution

2 引用 (Scopus)

抜粋

WISH is a new space science mission concept whose primary goal is to study the first galaxies in the early universe. We will launch a 1.5m telescope equipped with 1000 arcmin2 wide-field NIR camera by late 2010's in order to conduct unique ultra-deep and wide-area sky surveys at 1-5 micron. The primary science goal of WISH mission is pushing the high-redshift frontier beyond the epoch of reionization by utilizing its unique imaging capability and the dedicated survey strategy. We expect to detect ∼ 104 galaxies at z=8-9, ∼ 3-6×103 galaxies at z=11-12, and ∼50-100 galaxies at z=14-17 within about 5 years of the planned mission life time. It is worth mentioning that a large fraction of these objects may be bright enough for the spectroscopic observations with the extremely large telescopes. By adopting the optimized strategy for the recurrent observations to reach the depth, we also use the surveys to detect transient objects. Type Ia Supernova cosmology is thus another important primary goal of WISH. A unique optical layout has been developed to achieve the diffraction-limited imaging at 1-5micron over the required large area. Cooling the mirror and telescope to ∼100K is needed to achieve the zodiacal light limited imaging and WISH will achieve the required temperature by passive cooling in the stable thermal environment at the orbit near Sun-Earth L2. We are conducting the conceptual studies and development for the important components of WISH including the exchange mechanism for the wide-field filters as well as the primary mirror fixation.

元の言語English
ホスト出版物のタイトルSpace Telescopes and Instrumentation 2010
ホスト出版物のサブタイトルOptical, Infrared, and Millimeter Wave
DOI
出版物ステータスPublished - 2010
外部発表Yes
イベントSpace Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave - San Diego, CA, United States
継続期間: 2010 6 272010 7 2

出版物シリーズ

名前Proceedings of SPIE - The International Society for Optical Engineering
7731
ISSN(印刷物)0277-786X

Conference

ConferenceSpace Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
United States
San Diego, CA
期間10/6/2710/7/2

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

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    Yamada, T., Doi, M., Gotc, T., Ikeda, Y., Imanishi, M., Inoue, A., Iwamura, S., Iwata, I., Kawai, N., Kobayashie, M. A. R., Kodama, T., Komiyama, Y., Matsuhara, H., Matsuoka, Y., Morokuma, T., Ohta, K., Oyabu, S., Sato, Y., Sugita, H., ... Yonetoku, D. (2010). WISH: Wide-field imaging surveyor for high-redshift. : Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave [77311Q] (Proceedings of SPIE - The International Society for Optical Engineering; 巻数 7731). https://doi.org/10.1117/12.856561