TY - GEN
T1 - High-z gamma-ray bursts unraveling the dark ages and extreme space-time mission - HiZ-GUNDAM
AU - Wide Field X-ray Monitor Collaboration
AU - Near Infrared Telescope Collaboration
AU - Satellite System Collaboration
AU - Science Collaboration
AU - Follow-up Collaboration
AU - Yonetoku, Daisuke
AU - Doi, Akihiro
AU - Mihara, Tatehiro
AU - Matsuhara, Hideo
AU - Sakamoto, Takanori
AU - Tsumura, Kohji
AU - Ioka, Kunihito
AU - Arimoto, Makoto
AU - Enoto, Teruaki
AU - Fujimoto, Kenjiro
AU - Goto, Hatsune
AU - Gunji, Shuichi
AU - Hiraga, Junko
AU - Ikunaga, Shintaro
AU - Kawai, Nobuyuki
AU - Kondo, Ryuji
AU - Kurosawa, Shunsuke
AU - Li, Junyi
AU - Maeda, Yoshitomo
AU - Mitsuishi, Ikuyuki
AU - Murakami, Toshio
AU - Nagataka, Issin
AU - Nakagawa, Yujin
AU - Ogino, Naoki
AU - Owari, Taiki
AU - Sato, Ryuji
AU - Sato, Masataka
AU - Sato, Tomoya
AU - Sawano, Tatsuya
AU - Serino, Motoko
AU - Shen, Hsien Chieh
AU - Sugita, Satoshi
AU - Takahashi, Shuta
AU - Tamagawa, Toru
AU - Tamura, Keisuke
AU - Tanaka, Takaaki
AU - Tanimori, Toru
AU - Tashiro, Makoto S.
AU - Togashi, Takumi
AU - Tomida, Hiroshi
AU - Watanabe, Keito
AU - Yamaoka, Kazutaka
AU - Yamauchi, Makoto
AU - Yatsu, Yoichi
AU - Yoshida, Atsumasa
AU - Akitaya, Hiroshi
AU - Fukui, Akihiko
AU - Fukui, Haruki
AU - Ita, Yoshifusa
AU - Murase, Kohta
N1 - Publisher Copyright:
© 2024 SPIE.
PY - 2024
Y1 - 2024
N2 - HiZ-GUNDAM is a future satellite mission whose mission concept was approved by ISAS/JAXA, and it is one of the future satellite candidates of JAXA's competitive medium-class mission. HiZ-GUNDAM will lead time-domain astronomy in 2030s, and its key sciences are (1) exploration of the early universe with high-redshift gamma-ray bursts, and (2) contribution to the multi-messenger astronomy. Two mission payloads are aboard HiZ-GUNDAM to realize these two scientific issues. The wide field X-ray monitors which consist of Lobster Eye optics array and focal imaging sensor, monitor ~0.5 steradian field of view in 0.5-4 keV energy range. The near infrared telescope with an aperture size of 30 cm in diameter performs simultaneous 5-band photometric observation in 0.5-2.5 µm wavelength with Koester's prism for X-ray transients discovered by Wide Field X-ray Monitor. In this paper, we introduce the mission overview of HiZ-GUNDAM while the information contained herein may change in future studies.
AB - HiZ-GUNDAM is a future satellite mission whose mission concept was approved by ISAS/JAXA, and it is one of the future satellite candidates of JAXA's competitive medium-class mission. HiZ-GUNDAM will lead time-domain astronomy in 2030s, and its key sciences are (1) exploration of the early universe with high-redshift gamma-ray bursts, and (2) contribution to the multi-messenger astronomy. Two mission payloads are aboard HiZ-GUNDAM to realize these two scientific issues. The wide field X-ray monitors which consist of Lobster Eye optics array and focal imaging sensor, monitor ~0.5 steradian field of view in 0.5-4 keV energy range. The near infrared telescope with an aperture size of 30 cm in diameter performs simultaneous 5-band photometric observation in 0.5-2.5 µm wavelength with Koester's prism for X-ray transients discovered by Wide Field X-ray Monitor. In this paper, we introduce the mission overview of HiZ-GUNDAM while the information contained herein may change in future studies.
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U2 - 10.1117/12.3018571
DO - 10.1117/12.3018571
M3 - Conference contribution
AN - SCOPUS:85207646901
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - Space Telescopes and Instrumentation 2024
A2 - den Herder, Jan-Willem A.
A2 - Nikzad, Shouleh
A2 - Nakazawa, Kazuhiro
PB - SPIE
T2 - Space Telescopes and Instrumentation 2024: Ultraviolet to Gamma Ray
Y2 - 16 June 2024 through 21 June 2024
ER -