WISH for deep and wide NIR surveys

Toru Yamada; Ikuru Iwata; Makiko Ando; Mamoru Doi; Tomotsugu Goto; Yuji Ikeda; Masatoshi Imanishi; Akio K. Inoue; Satoru Iwamura; Nobuyuki Kawai; Masakazu A.R. Kobayashi; Tadayuki Kodama; Yutaka Komiyama; Mariko Kubo; Hideo Matsuhara; Ken Mawatari; Yoshiki Matsuoka; Tomoki Morokuma; Hidehiko Nakaya; Kouji Ohta; Atsushi Okamoto; Sinki Oyabu; Yoichi Sato; Hiroyuki Sugita; Ryo Tsutsui; Chihiro Tokoku; Jun Toshikawa; Saku Tsuneta; Takehiko Wada; Kiyoto Yabe; Naoki Yasuda; Daisuke Yonetoku

doi:10.1117/12.925632

WISH for deep and wide NIR surveys

Toru Yamada, Ikuru Iwata, Makiko Ando, Mamoru Doi, Tomotsugu Goto, Yuji Ikeda, Masatoshi Imanishi, Akio K. Inoue, Satoru Iwamura, Nobuyuki Kawai, Masakazu A.R. Kobayashi, Tadayuki Kodama, Yutaka Komiyama, Mariko Kubo, Hideo Matsuhara, Ken Mawatari, Yoshiki Matsuoka, Tomoki Morokuma, Hidehiko Nakaya, Kouji OhtaAtsushi Okamoto, Sinki Oyabu, Yoichi Sato, Hiroyuki Sugita, Ryo Tsutsui, Chihiro Tokoku, Jun Toshikawa, Saku Tsuneta, Takehiko Wada, Kiyoto Yabe, Naoki Yasuda, Daisuke Yonetoku

SCI - Astronomy

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

8 Citations (Scopus)

Abstract

WISH, Wide-field Imaging Surveyor for High-redshiftt, is a space mission concept to conduct very deep and widefield surveys at near infrared wavelength at 1-5μm to study the properties of galaxies at very high redshift beyond the epoch of cosmic reionization. The concept has been developed and studied since 2008 to be proposed for future JAXA/ISAS mission. WISH has a 1.5m-diameter primary mirror and a wide-field imager covering 850 arcmin². The pixel scale is 0.155 arcsec for 18μm pitch, which properly samples the diffraction-limited image at 1.5μm. The main program is Ultra Deep Survey (UDS) covering 100 deg² down to 28AB mag at least in five broad bands. We expect to detect >10⁴ galaxies at z=8-9, 10 ³-10⁴ galaxies at z=11-12, and 50-100 galaxies at z>14, many of which can be feasible targets for deep spectroscopy with Extremely Large Telescopes. With recurrent deep observations, detection and light curve monitoring for type-Ia SNe in rest-frame infrared wavelength is also conducted, which is another main science goal of the mission. During the in-orbit 5 years observations, we expect to detect and monitor >2000 type-Ia SNe up to z̃2. WISH also conducts Ultra Wide Survey, covering 1000deg² down to 24-25AB mag as well as Extreme Survey, covering a limited number of fields of view down to 29-30AB mag. We here report the progress of the WISH project including the basic telescope and satellite design as well as the results of the test for a proto-model of the flip-type filter exchanger which works robustly near 100K.

Original language	English
Title of host publication	Space Telescopes and Instrumentation 2012
Subtitle of host publication	Optical, Infrared, and Millimeter Wave
DOIs	https://doi.org/10.1117/12.925632
Publication status	Published - 2012
Event	Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave - Amsterdam, Netherlands Duration: 2012 Jul 1 → 2012 Jul 6

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	8442
ISSN (Print)	0277-786X

Other

Other	Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave
Country/Territory	Netherlands
City	Amsterdam
Period	12/7/1 → 12/7/6

Keywords

Cosmology
Galaxies
Galaxy formation
Infrared
Space telescopes
Wide-field

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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10.1117/12.925632

Cite this

Yamada, T., Iwata, I., Ando, M., Doi, M., Goto, T., Ikeda, Y., Imanishi, M., Inoue, A. K., Iwamura, S., Kawai, N., Kobayashi, M. A. R., Kodama, T., Komiyama, Y., Kubo, M., Matsuhara, H., Mawatari, K., Matsuoka, Y., Morokuma, T., Nakaya, H., ... Yonetoku, D. (2012). WISH for deep and wide NIR surveys. In Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave [84421A] (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 8442). https://doi.org/10.1117/12.925632

Yamada, T, Iwata, I, Ando, M, Doi, M, Goto, T, Ikeda, Y, Imanishi, M, Inoue, AK, Iwamura, S, Kawai, N, Kobayashi, MAR, Kodama, T, Komiyama, Y, Kubo, M, Matsuhara, H, Mawatari, K, Matsuoka, Y, Morokuma, T, Nakaya, H, Ohta, K, Okamoto, A, Oyabu, S, Sato, Y, Sugita, H, Tsutsui, R, Tokoku, C, Toshikawa, J, Tsuneta, S, Wada, T, Yabe, K, Yasuda, N & Yonetoku, D 2012, WISH for deep and wide NIR surveys. in Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave., 84421A, Proceedings of SPIE - The International Society for Optical Engineering, vol. 8442, Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave, Amsterdam, Netherlands, 12/7/1. https://doi.org/10.1117/12.925632

@inproceedings{d120846350fb4b248d2be159fdcccad5,

title = "WISH for deep and wide NIR surveys",

abstract = "WISH, Wide-field Imaging Surveyor for High-redshiftt, is a space mission concept to conduct very deep and widefield surveys at near infrared wavelength at 1-5μm to study the properties of galaxies at very high redshift beyond the epoch of cosmic reionization. The concept has been developed and studied since 2008 to be proposed for future JAXA/ISAS mission. WISH has a 1.5m-diameter primary mirror and a wide-field imager covering 850 arcmin2. The pixel scale is 0.155 arcsec for 18μm pitch, which properly samples the diffraction-limited image at 1.5μm. The main program is Ultra Deep Survey (UDS) covering 100 deg2 down to 28AB mag at least in five broad bands. We expect to detect >104 galaxies at z=8-9, 10 3-104 galaxies at z=11-12, and 50-100 galaxies at z>14, many of which can be feasible targets for deep spectroscopy with Extremely Large Telescopes. With recurrent deep observations, detection and light curve monitoring for type-Ia SNe in rest-frame infrared wavelength is also conducted, which is another main science goal of the mission. During the in-orbit 5 years observations, we expect to detect and monitor >2000 type-Ia SNe up to {\~z}2. WISH also conducts Ultra Wide Survey, covering 1000deg2 down to 24-25AB mag as well as Extreme Survey, covering a limited number of fields of view down to 29-30AB mag. We here report the progress of the WISH project including the basic telescope and satellite design as well as the results of the test for a proto-model of the flip-type filter exchanger which works robustly near 100K.",

keywords = "Cosmology, Galaxies, Galaxy formation, Infrared, Space telescopes, Wide-field",

author = "Toru Yamada and Ikuru Iwata and Makiko Ando and Mamoru Doi and Tomotsugu Goto and Yuji Ikeda and Masatoshi Imanishi and Inoue, {Akio K.} and Satoru Iwamura and Nobuyuki Kawai and Kobayashi, {Masakazu A.R.} and Tadayuki Kodama and Yutaka Komiyama and Mariko Kubo and Hideo Matsuhara and Ken Mawatari and Yoshiki Matsuoka and Tomoki Morokuma and Hidehiko Nakaya and Kouji Ohta and Atsushi Okamoto and Sinki Oyabu and Yoichi Sato and Hiroyuki Sugita and Ryo Tsutsui and Chihiro Tokoku and Jun Toshikawa and Saku Tsuneta and Takehiko Wada and Kiyoto Yabe and Naoki Yasuda and Daisuke Yonetoku",

year = "2012",

doi = "10.1117/12.925632",

language = "English",

isbn = "9780819491435",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

booktitle = "Space Telescopes and Instrumentation 2012",

note = "Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave ; Conference date: 01-07-2012 Through 06-07-2012",

}

TY - GEN

T1 - WISH for deep and wide NIR surveys

AU - Yamada, Toru

AU - Iwata, Ikuru

AU - Ando, Makiko

AU - Doi, Mamoru

AU - Goto, Tomotsugu

AU - Ikeda, Yuji

AU - Imanishi, Masatoshi

AU - Inoue, Akio K.

AU - Iwamura, Satoru

AU - Kawai, Nobuyuki

AU - Kobayashi, Masakazu A.R.

AU - Kodama, Tadayuki

AU - Komiyama, Yutaka

AU - Kubo, Mariko

AU - Matsuhara, Hideo

AU - Mawatari, Ken

AU - Matsuoka, Yoshiki

AU - Morokuma, Tomoki

AU - Nakaya, Hidehiko

AU - Ohta, Kouji

AU - Okamoto, Atsushi

AU - Oyabu, Sinki

AU - Sato, Yoichi

AU - Sugita, Hiroyuki

AU - Tsutsui, Ryo

AU - Tokoku, Chihiro

AU - Toshikawa, Jun

AU - Tsuneta, Saku

AU - Wada, Takehiko

AU - Yabe, Kiyoto

AU - Yasuda, Naoki

AU - Yonetoku, Daisuke

PY - 2012

Y1 - 2012

N2 - WISH, Wide-field Imaging Surveyor for High-redshiftt, is a space mission concept to conduct very deep and widefield surveys at near infrared wavelength at 1-5μm to study the properties of galaxies at very high redshift beyond the epoch of cosmic reionization. The concept has been developed and studied since 2008 to be proposed for future JAXA/ISAS mission. WISH has a 1.5m-diameter primary mirror and a wide-field imager covering 850 arcmin2. The pixel scale is 0.155 arcsec for 18μm pitch, which properly samples the diffraction-limited image at 1.5μm. The main program is Ultra Deep Survey (UDS) covering 100 deg2 down to 28AB mag at least in five broad bands. We expect to detect >104 galaxies at z=8-9, 10 3-104 galaxies at z=11-12, and 50-100 galaxies at z>14, many of which can be feasible targets for deep spectroscopy with Extremely Large Telescopes. With recurrent deep observations, detection and light curve monitoring for type-Ia SNe in rest-frame infrared wavelength is also conducted, which is another main science goal of the mission. During the in-orbit 5 years observations, we expect to detect and monitor >2000 type-Ia SNe up to z̃2. WISH also conducts Ultra Wide Survey, covering 1000deg2 down to 24-25AB mag as well as Extreme Survey, covering a limited number of fields of view down to 29-30AB mag. We here report the progress of the WISH project including the basic telescope and satellite design as well as the results of the test for a proto-model of the flip-type filter exchanger which works robustly near 100K.

AB - WISH, Wide-field Imaging Surveyor for High-redshiftt, is a space mission concept to conduct very deep and widefield surveys at near infrared wavelength at 1-5μm to study the properties of galaxies at very high redshift beyond the epoch of cosmic reionization. The concept has been developed and studied since 2008 to be proposed for future JAXA/ISAS mission. WISH has a 1.5m-diameter primary mirror and a wide-field imager covering 850 arcmin2. The pixel scale is 0.155 arcsec for 18μm pitch, which properly samples the diffraction-limited image at 1.5μm. The main program is Ultra Deep Survey (UDS) covering 100 deg2 down to 28AB mag at least in five broad bands. We expect to detect >104 galaxies at z=8-9, 10 3-104 galaxies at z=11-12, and 50-100 galaxies at z>14, many of which can be feasible targets for deep spectroscopy with Extremely Large Telescopes. With recurrent deep observations, detection and light curve monitoring for type-Ia SNe in rest-frame infrared wavelength is also conducted, which is another main science goal of the mission. During the in-orbit 5 years observations, we expect to detect and monitor >2000 type-Ia SNe up to z̃2. WISH also conducts Ultra Wide Survey, covering 1000deg2 down to 24-25AB mag as well as Extreme Survey, covering a limited number of fields of view down to 29-30AB mag. We here report the progress of the WISH project including the basic telescope and satellite design as well as the results of the test for a proto-model of the flip-type filter exchanger which works robustly near 100K.

KW - Cosmology

KW - Galaxies

KW - Galaxy formation

KW - Infrared

KW - Space telescopes

KW - Wide-field

UR - http://www.scopus.com/inward/record.url?scp=84871843690&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84871843690&partnerID=8YFLogxK

U2 - 10.1117/12.925632

DO - 10.1117/12.925632

M3 - Conference contribution

AN - SCOPUS:84871843690

SN - 9780819491435

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Space Telescopes and Instrumentation 2012

T2 - Space Telescopes and Instrumentation 2012: Optical, Infrared, and Millimeter Wave

Y2 - 1 July 2012 through 6 July 2012

ER -

WISH for deep and wide NIR surveys

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