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The challenge of identifying Galactic TeV sources
https://jaxa.repo.nii.ac.jp/records/5297
https://jaxa.repo.nii.ac.jp/records/52974429af72-4e10-47f1-b174-987482f2953c
| 名前 / ファイル | ライセンス | アクション |
|---|---|---|
64306058.pdf (400.3 kB)
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| Item type | 会議発表論文 / Conference Paper(1) | |||||||
|---|---|---|---|---|---|---|---|---|
| 公開日 | 2015-03-26 | |||||||
| タイトル | ||||||||
| タイトル | The challenge of identifying Galactic TeV sources | |||||||
| 言語 | en | |||||||
| 言語 | ||||||||
| 言語 | eng | |||||||
| キーワード | ||||||||
| 言語 | en | |||||||
| 主題Scheme | Other | |||||||
| 主題 | astrophysics : high-energy - observations : TeV, X-rays - source identification techniques | |||||||
| 資源タイプ | ||||||||
| 資源タイプ識別子 | http://purl.org/coar/resource_type/c_5794 | |||||||
| 資源タイプ | conference paper | |||||||
| 著者 |
Reimer, Olaf
× Reimer, Olaf
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| 著者所属（英） | ||||||||
| en | ||||||||
| W.W.Hansen Experimental Physics Laboratory & Kavli Institute for Particle Astrophysics and Cosmology, Stanford University | ||||||||
| 出版者 | ||||||||
| 出版者 | 宇宙航空研究開発機構 | |||||||
| 出版者（英） | ||||||||
| 出版者 | Japan Aerospace Exploration Agency (JAXA) | |||||||
| 書誌情報 |
宇宙航空研究開発機構特別資料 en : JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop 巻 JAXA-SP-08-014E, p. 294-299, 発行日 2009-02-27 |
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| 会議概要（会議名, 開催地, 会期, 主催者等）（英） | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008) | |||||||
| 抄録（英） | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | Since VHE gamma-ray observations made during the H.E.S.S. Galactic Plane Survey revealed for the first time the existence of dozens of extreme particle accelerators in our Galaxy, source identification became a crucial aspect in ground-based high-energy gamma-ray astronomy. Whereas the general problem resembles that of the unidentified EGRET sources, a low-threshold imaging Cherenkov telescope array's superior angular resolution and resulting imaging capability against a drastically reduced diffuse component enables different identification techniques. Given that IC photons at TeV energies originate from seed photons at keV energies, the wide field X-ray imaging capabilities and high duty cycle of the MAXI mission will provide contemporaneous X-ray observations to essentially all VHE gamma-ray observations to come, and might ultimately help to characterize the underlying particle population of these extreme Galactic gamma-ray emitter. Most particular, the so far sparsely probed domain of time dependent high-energy characteristics offered from all-sky monitoring by MAXI will add new perspectives to the exploration of VHE gamma-ray sources. | |||||||
| 内容記述（英） | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | Physical characteristics: Original contains color illustrations | |||||||
| ISSN | ||||||||
| 収録物識別子タイプ | ISSN | |||||||
| 収録物識別子 | 1349-113X | |||||||
| 書誌レコードID | ||||||||
| 収録物識別子タイプ | NCID | |||||||
| 収録物識別子 | AA11984031 | |||||||
| 資料番号 | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | 資料番号: AA0064306058 | |||||||
| レポート番号 | ||||||||
| 内容記述タイプ | Other | |||||||
| 内容記述 | レポート番号: JAXA-SP-08-014E | |||||||
