High-z gamma-ray bursts unraveling the dark ages and extreme space-time mission: HiZ-GUNDAM
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- Jan-Willem A. den Herder
- editor
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- Kazuhiro Nakazawa
- editor
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- Shouleh Nikzad
- editor
説明
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.
収録刊行物
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- Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray
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Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray 11444 114442Z-, 2020-12-13
SPIE
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詳細情報 詳細情報について
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- CRID
- 1360009142678875776
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- 資料種別
- journal article
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- データソース種別
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- Crossref
- KAKEN
- OpenAIRE