2015 Fiscal Year Final Research Report
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 |
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| Section | 一般 |
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| Research Field |
Astronomy
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| Research Institution | Aoyama Gakuin University |
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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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| Keywords | 高エネルギー天体 / 時間変動天体 / X線 / ガンマ線 |
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| 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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| Free Research Field |
高エネルギー突発天体現象
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