Study of time-domain astronomical sources using the MAXI and the Swift data
Project/Area Number |
25400234
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Research Category |
Grant-in-Aid for Scientific Research (C)
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Allocation Type | Multi-year Fund |
Section | 一般 |
Research Field |
Astronomy
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Research Institution | Aoyama Gakuin University |
Principal Investigator |
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Research Collaborator |
ODA Yuma 青山学院大学, 理工学部, 学生
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Project Period (FY) |
2013-04-01 – 2016-03-31
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Project Status |
Completed (Fiscal Year 2015)
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Budget Amount *help |
¥4,420,000 (Direct Cost: ¥3,400,000、Indirect Cost: ¥1,020,000)
Fiscal Year 2015: ¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
Fiscal Year 2014: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2013: ¥1,820,000 (Direct Cost: ¥1,400,000、Indirect Cost: ¥420,000)
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Keywords | 高エネルギー天体 / 時間変動天体 / X線 / ガンマ線 / 高エネルギー宇宙物理学 / 突発天体 |
Outline of Final Research Achievements |
Our research goal is to construct a broad-band transient monitor from 2 keV up to 200 keV to lead an exciting field of time-domain astronomy here in Japan. We newly developed the automatic pipeline to analyze the MAX (International Space Station's mission) and the Swift (NASA gamma-ray burst explorer mission) data to construct broad-band light curves of 106 bright hard X-ray sources. The light curves are publicly available from the web server.
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Report
(4 results)
Research Products
(3 results)
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[Journal Article] Swift/BAT and MAXI/GSC Broadband Transient Monitor2016
Author(s)
Sakamoto, T., Oda, R., Mihara, T., Yoshida, A., Arimoto, M., Barthelmy, S., Kawai, N., Krimm, H., Nakahira, S., Serino, M.
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Journal Title
Publication of Astronomical Society of Japan
Volume: 01
Issue: SP1
Pages: 01-01
DOI
Related Report
Peer Reviewed / Open Access / Int'l Joint Research / Acknowledgement Compliant
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