High-redshift gamma-ray burst for unraveling the Dark Ages Mission: HiZ-GUNDAM
High-redshift gamma-ray burst for unraveling the Dark Ages Mission: HiZ-GUNDAM
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DOI：
10.1117/12.2560603
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发表时间：
2020-12
期刊：
影响因子：
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通讯作者：
D. Yonetoku;T. Mihara;A. Doi;T. Sakamoto;K. Tsumura;K. Ioka;Yusuke Amaya;M. Arimoto;T. Enoto;Takeru Fujii;Hatsune Goto;S. Gunji;J. Hiraga;H. Ikeda;N. Kawai;S. Kurosawa;Jin Li;Y. Maeda;I. Mitsuishi;T. Murakami;Y. Nakagawa;N. Ogino;M. Ohno;T. Sawano;Kensyo Sei;M. Serino;S. Sugita;T. Tamagawa;K. Tamura;Takaaki Tanaka;T. Tanimori;M. Tashiro;H. Tomida;Hyeongsoon Wang;Tomohiro Yamaguchi;A. Yamamoto;K. Yamaoka;M. Yamauchi;Y. Yatsu;A. Yoshida;D. Yuhi;H. Akitaya;A. Fukui;Y. Ita;H. Kaneda;K. Kawabata;Yoshikatsu Kawata;Miku Kurimata;T. Matsumoto;S. Matsuura;A. Miyasaka;K. Motohara;N. Narita;H. Noda;A. Ohashi;H. Okita;K. Sano;Masaomi Tanaka;Y. Urata;T. Wada;H. Yamaguchi;K. Yanagisawa;Michitoshi Yoshida;K. Asano;K. Inayoshi;S. Inoue;Hirotaka Ito;H. Izumiura;N. Kawanaka;T. Kinugawa;S. Kisaka;K. Kiuchi;J. Matsumoto;A. Mizuta;K. Murase;H. Nagakura;S. Nagataki;Y. Nakada;Takashi Nakamura;Y. Niino;Y. Suwa;Keitaro Takahashi;Takahiro Tanaka;K. Toma;T. Totani;R. Yamazaki;J. Yokoyama
中科院分区：
文献类型：
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作者：
D. Yonetoku;T. Mihara;A. Doi;T. Sakamoto;K. Tsumura;K. Ioka;Yusuke Amaya;M. Arimoto;T. Enoto;Takeru Fujii;Hatsune Goto;S. Gunji;J. Hiraga;H. Ikeda;N. Kawai;S. Kurosawa;Jin Li;Y. Maeda;I. Mitsuishi;T. Murakami;Y. Nakagawa;N. Ogino;M. Ohno;T. Sawano;Kensyo Sei;M. Serino;S. Sugita;T. Tamagawa;K. Tamura;Takaaki Tanaka;T. Tanimori;M. Tashiro;H. Tomida;Hyeongsoon Wang;Tomohiro Yamaguchi;A. Yamamoto;K. Yamaoka;M. Yamauchi;Y. Yatsu;A. Yoshida;D. Yuhi;H. Akitaya;A. Fukui;Y. Ita;H. Kaneda;K. Kawabata;Yoshikatsu Kawata;Miku Kurimata;T. Matsumoto;S. Matsuura;A. Miyasaka;K. Motohara;N. Narita;H. Noda;A. Ohashi;H. Okita;K. Sano;Masaomi Tanaka;Y. Urata;T. Wada;H. Yamaguchi;K. Yanagisawa;Michitoshi Yoshida;K. Asano;K. Inayoshi;S. Inoue;Hirotaka Ito;H. Izumiura;N. Kawanaka;T. Kinugawa;S. Kisaka;K. Kiuchi;J. Matsumoto;A. Mizuta;K. Murase;H. Nagakura;S. Nagataki;Y. Nakada;Takashi Nakamura;Y. Niino;Y. Suwa;Keitaro Takahashi;Takahiro Tanaka;K. Toma;T. Totani;R. Yamazaki;J. Yokoyama
HiZ-GUNDAM是一个未来的卫星使命，它将通过观测高能瞬态现象来引领时域天文学和多信使天文学。HiZ-GUNDAM的使命概念得到了ISAS/JAXA的批准，它是JAXA中级使命的未来候选卫星之一。我们正处于预阶段A（项目前），并详细阐述了使命概念，使命/系统要求，以便在21世纪20年代末发射。HiZ-GUNDAM使命的主要任务是：（1）利用高红移伽玛射线暴探索早期宇宙;（2）对多信使天文学的贡献。HiZ-GUNDAM有两种使命有效载荷。宽视场X射线监视器由龙虾眼光学阵列和聚焦成像传感器组成，在0.5 - 4 keV能量范围内监视~1球面度视场。近红外望远镜的孔径尺寸为直径30厘米，可同时观测0.5 - 2.5 μm之间的四个波段。在本文中，我们介绍了HiZ-GUNDAM的使命概述。
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.