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26 August 2022 High-redshift gamma-ray burst for unraveling the dark ages Mmission: HiZ-GUNDAM
Daisuke Yonetoku, Akihiro Doi, Tatehiro Mihara, Takanori Sakamoto, Kohji Tsumura, Makoto Arimoto, Tatsuya Sawano, Shuichi Gunji
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Proceedings Volume 12181, Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray; 121811J (2022) https://doi.org/10.1117/12.2629179
Event: SPIE Astronomical Telescopes + Instrumentation, 2022, Montréal, Québec, Canada
Abstract
HiZ-GUNDAM is a candidate of future satellite mission for the Japanese competitive M-class mission by ISAS/JAXA to progress a time-domain astronomy and multi-messenger astronomy with gamma-ray burst (GRB) phenomena. The science goals are (1) to probe the early universe with high redshift GRBs at z > 7, and (2) to promote the gravitational wave astronomy with short GRB. HiZ-GUNDAM has been successfully passed a review for pre-project candidate in November 2021, and its team is working on the concept study. We will introduce the sciences and mission overview of HiZ-GUNDAM.
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Daisuke Yonetoku, Akihiro Doi, Tatehiro Mihara, Takanori Sakamoto, Kohji Tsumura, Makoto Arimoto, Tatsuya Sawano, and Shuichi Gunji "High-redshift gamma-ray burst for unraveling the dark ages Mmission: HiZ-GUNDAM", Proc. SPIE 12181, Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray, 121811J (26 August 2022); https://doi.org/10.1117/12.2629179
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KEYWORDS
Gamma radiation
Astronomy
Gamma-ray astronomy
X-ray imaging
X-ray optics
Satellites
Sensors
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