TY - GEN
T1 - High-redshift gamma-ray burst for unraveling the Dark Ages Mission - HiZ-GUNDAM -
AU - Wide Field X-ray Monitor Collaboration
AU - Near Infrared Telescope Collaboration
AU - Science Collaboration
AU - Yonetoku, Daisuke
AU - Mihara, Tatehiro
AU - Doi, Akihiro
AU - Sakamoto, Takanori
AU - Tsumura, Kohji
AU - Ioka, Kunihito
AU - Amaya, Yusuke
AU - Arimoto, Makoto
AU - Enoto, Teruaki
AU - Fujii, Takeru
AU - Goto, Hatsune
AU - Gunji, Shuichi
AU - Hiraga, Junko
AU - Ikeda, Hirokazu
AU - Kawai, Nobuyuki
AU - Kurosawa, Shunsuke
AU - Li, Jin
AU - Maeda, Yoshitomo
AU - Mitsuishi, Ikuyuki
AU - Murakami, Toshio
AU - Nakagawa, Yujin
AU - Ogino, Naoki
AU - Ohno, Masanori
AU - Sawano, Tatsuya
AU - Sei, Kensyo
AU - Serino, Motoko
AU - Sugita, Satoshi
AU - Tamagawa, Toru
AU - Tamura, Keisuke
AU - Tanaka, Takaaki
AU - Tanimori, Toru
AU - Tashiro, Makoto S.
AU - Tomida, Hiroshi
AU - Wang, Hyeongsoon
AU - Yamaguchi, Tomohiro
AU - Yamamoto, Ayumi
AU - Yamaoka, Kazutaka
AU - Yamauchi, Makoto
AU - Yatsu, Yoichi
AU - Yoshida, Atsumasa
AU - Yuhi, Daito
AU - Akitaya, Hiroshi
AU - Fukui, Akihiko
AU - Ita, Yoshifusa
AU - Kaneda, Hidehiro
AU - Kawabata, Koji
AU - Kawata, Yoshikatsu
AU - Kurimata, Miku
AU - Tanaka, Masaomi
AU - Toma, Kenji
N1 - Funding Information:
This research was supported by JSPS KAKENHI Grant Numbers 16H06342 (DY), 15H00780 (DY), 18H04580 (DY), and Aerospace Science and Technology Promotion commission expenses (DY), and Sakigake project 2018 of Kanazawa University.
Publisher Copyright:
© 2020 SPIE
PY - 2020
Y1 - 2020
N2 - HiZ-GUNDAM is a future satellite mission which will lead the time-domain astronomy and the multi-messenger astronomy through observations of high-energy transient phenomena. A mission concept of HiZ-GUNDAM was approved by ISAS/JAXA, and it is one of the future satellite candidates of JAXA's medium-class mission. We are in pre-phase A (before pre-project) and elaborating the mission concept, mission/system requirements for the launch in the late 2020s. The main themes of HiZ-GUNDAM mission are (1) exploration of the early universe with high-redshift gamma-ray bursts, and (2) contribution to the multi-messenger astronomy. HiZ-GUNDAM has two kinds of mission payload. The wide field X-ray monitors consist of Lobster Eye optics array and focal imaging sensor, and monitor ~1 steradian field of view in 0.5 - 4 keV energy range. The near infrared telescope has an aperture size 30 cm in diameter, and simultaneously observes four wavelength bands between 0.5 - 2.5 µm. In this paper, we introduce the mission overview of HiZ-GUNDAM.
AB - HiZ-GUNDAM is a future satellite mission which will lead the time-domain astronomy and the multi-messenger astronomy through observations of high-energy transient phenomena. A mission concept of HiZ-GUNDAM was approved by ISAS/JAXA, and it is one of the future satellite candidates of JAXA's medium-class mission. We are in pre-phase A (before pre-project) and elaborating the mission concept, mission/system requirements for the launch in the late 2020s. The main themes of HiZ-GUNDAM mission are (1) exploration of the early universe with high-redshift gamma-ray bursts, and (2) contribution to the multi-messenger astronomy. HiZ-GUNDAM has two kinds of mission payload. The wide field X-ray monitors consist of Lobster Eye optics array and focal imaging sensor, and monitor ~1 steradian field of view in 0.5 - 4 keV energy range. The near infrared telescope has an aperture size 30 cm in diameter, and simultaneously observes four wavelength bands between 0.5 - 2.5 µm. In this paper, we introduce the mission overview of HiZ-GUNDAM.
KW - Astronomical satellite
KW - Early universe
KW - Gamma-ray bursts
KW - Multi-messenger astronomy
KW - Near infrared
KW - X-ray
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U2 - 10.1117/12.2560603
DO - 10.1117/12.2560603
M3 - Conference contribution
AN - SCOPUS:85099316218
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2020
A2 - den Herder, Jan-Willem A.
A2 - Nikzad, Shouleh
A2 - Nakazawa, Kazuhiro
PB - SPIE
T2 - Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
Y2 - 14 December 2020 through 18 December 2020
ER -