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チェレンコフ宇宙ガンマ線グループ(CTAグループ)
Showing the original Japanese · View translation
超高エネルギーのガンマ線で、激しい宇宙の姿をとらえる研究室。

AboutAbout the lab
いちばん高いエネルギーの光で宇宙を見る。
チェレンコフ宇宙ガンマ線グループは、
ガンマ線は
大気に
次世代の
Key terms
- ガンマ線
- 電磁波の
うちでもっとも エネルギーの 高い もの。 激しい 天体現象から 放たれる - チェレンコフ光
- 高速の
荷電粒子が 大気の 中を 走る ときに 出る光。 重なり合って 短い フラッシュに なる - 暗黒物質
- 宇宙を
満たしていながら、 光では 見る ことのできない正体 不明の 物質
NewsLab news
学振特別研究員が、
日本物理学会 若手奨 励賞を 受賞 博士課程と
修士課程の 学生が、 日本物理学会 学生優秀発表賞を 受賞 研究員が、
Werner Hofmann Scientific Award を 受賞 博士課程の
学生が、 宇宙線研究所の 研究発表会で 所長賞を 受賞 博士課程の
学生が、 日本物理学会 年次大会で 学生優秀発表賞を 受賞
ResearchResearch themes
大気チェレンコフ望遠鏡に
*Illustrative image高エネルギー天体の観測
超新星残骸、
*Illustrative image粒子加速と宇宙線の起源
高エネルギー天体で
*Illustrative image星と銀河の形成史
遠くから
*Illustrative image暗黒物質の探査
暗黒物質どうしが
MembersFaculty
チェレンコフ宇宙ガンマ線グループの
- Professor窪 秀利Publications ↗
- Project Professorマジン ダニエル
- Associate Professor齋藤 隆之Publications ↗
- Associate Professor奥村 曉Publications ↗
- Associate Professorホフク イブゲンPublications ↗
- Assistant Professor野崎 誠也Publications ↗
- Assistant Professor大石 理子Publications ↗
- Assistant Professor辻 直美
- Project Assistant Professorストゥルース マーセルPublications ↗
- Project Assistant Professor髙橋 光成
VoicesStudent voices
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On a 4-point scale, ● marks where students' answers fall
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RelatedLabs similar to チェレンコフ宇宙ガンマ線グループ(CTAグループ)
The information on this page is compiled by the LabLog team from the lab's public information and interviews. For corrections or removal requests, please contact LabLog, not the lab.
Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Roque de los Muchachos - ORM - MAGIC I” H. Zell / CC BY-SA 3.0 (cropped)
- 高エネルギー天体の
観測: “The Crab Nebula (weic2326a)” NASA, ESA, CSA, STScI, T. Temim (Princeton University) / CC BY 4.0 (cropped) - 粒子加速と
宇宙線の 起源: “Vela supernova - VST - Eso2214a” ESO/TIMER survey / CC BY 4.0 (cropped) - 星と
銀河の 形成史: “Hubble ultra deep field” NASA and the European Space Agency / Public domain (cropped) - 暗黒物質の
探査: “Center of the Milky Way Galaxy IV – Composite” NASA/JPL-Caltech/ESA/CXC/STScI / Public domain (cropped) - Related lab (Liang研究室): “NuclideMap stitched 2” NuclideMap.PNG: The viewer derivative work: Neokortex (talk) / Public domain (cropped)
- Related lab (安東研究室): “NS binary merger simulation 323” NASA/AEI/ZIB/M. Koppitz and L. Rezzolla / Public domain (cropped)
- Related lab (馬場研究室): “Supernova Remnant SN 1006” X-ray: NASA/CXC/Rutgers/G.Cassam-Chenaï, J.Hughes et al.; Radio: NRAO/AUI/NSF/GBT/VLA/Dyer, Maddalena & Cornwell; Optical: Middlebury College/F.Winkler, NOAO/AURA/NSF/CTIO Schmidt & DSS / CC BY 4.0 (cropped)
- Related lab (Cannon研究室): “Maya-NR-Simulation-with-Waveform-frame788” Deborah Ferguson ほか、
Georgia Tech MAYA Collaboration / CC BY-SA 4.0 (cropped)
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Learn more about LabLog ↗Search engines and AI may reference the basic lab info and rating summaries on this page and the description of LabLog. Student voices are for student members only. Automated collection by programs (scraping, or input to or training of AI) is prohibited under Article 8 of the Terms of Service. If you need data for research or analysis, please contact us.



