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 - Matsumoto, Toshio
AU - Murase, Kohta
N1 - 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.
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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 -