OPTICAL-INFRARED AND HIGH-ENERGY ASTRONOMY COLLABORATION AT HIROSHIMA ASTROPHYSICAL SCIENCE CENTER
OPTICAL-INFRARED AND HIGH-ENERGY ASTRONOMY COLLABORATION AT HIROSHIMA ASTROPHYSICAL SCIENCE CENTER
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广岛天体物理科学中心的光红外和高能天文学合作
DOI：
10.5303/pkas.2015.30.2.679
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发表时间：
2015
期刊：
影响因子：
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通讯作者：
T. Nakaoka
中科院分区：
文献类型：
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作者：
M. Uemura;Michitoshi Yoshida;K. Kawabata;T. Mizuno;Yasuyuki T. Tanaka;H. Akitaya;Y. Utsumi;Y. Moritani;R. Itoh;Y. Fukazawa;H. Takahashi;M. Ohno;T. Ui;K. Takaki;N. Ebisuda;K. Kawaguchi;K. Mori;Y. Ohashi;Y. Kanda;M. Kawabata;K. Takata;T. Nakaoka
广岛天体物理科学中心（HASC）于2004年在日本广岛大学成立。该研究所的主要使命是通过多波长观测对各种瞬变天体进行观测研究，包括伽马射线暴、超新星、新星、激变变星和活动星系核。HASC由三个部门组成：光学-红外天文学部门，高能天文学部门和理论天文学部门。哈萨克斯坦航天中心正在操作1.5米光学红外望远镜金田，该望远镜专门用于对瞬变物体进行跟踪和监测观测。高能区是费米伽马射线太空望远镜的关键操作中心。HASC和广岛大学物理科学系的高能天文学小组正在密切合作，以促进多波长时域天文学。我们报告的HASC和一些科学主题追求这个多波长合作的最新活动。
The Hiroshima Astrophysical Science Center (HASC) was founded in 2004 at Hiroshima University, Japan. The main mission of this institute is the observational study of various transient objects including gamma-ray bursts, supernovae, novae, cataclysmic variables, and active galactic nuclei by means of multi-wavelength observations. HASC consists of three divisions; the optical-infrared astronomy division, high-energy astronomy division, and theoretical astronomy division. HASC is operating the 1.5m optical-infrared telescope Kanata, which is dedicated to follow-up and monitoring observations of transient objects. The high-energy division is the key operation center for the Fermi gamma-ray space telescope. HASC and the high-energy astronomy group in the department of physical science at Hiroshima University are closely collaborating with each other to promote multi-wavelength time-domain astronomy. We report the recent activities of HASC and some science topics pursued by this multi-wavelength collaboration.