LAB LOGA page on LabLog, a review site (not the lab's official page)
森下 貴弘 研究室
Showing the original Japanese · View translation
初期宇宙の銀河の成り立ちを望遠鏡の観測で探る研究室。
AboutAbout the lab
初期宇宙の銀河を、観測で読み解く。
森下貴弘研究室は、
ハッブル宇宙望遠鏡と
研究テーマは、
ローマン宇宙望遠鏡の
Key terms
- 宇宙再電離
- 宇宙の
初期に 中性だった 水素ガスが、 天体の 光に よって 再び電離した 現象。 その 時代の 銀河を 調べる - 原始銀河団
- 銀河団が
できる 前の 段階で、 銀河が 集まり 始めている 領域 - JWST
- ジェイムズ・ウェッブ宇宙望遠鏡の
略称。 赤外線で 遠方の 宇宙を 観測する 宇宙望遠鏡 - 化学進化
- 銀河の
中で 星が 生まれ死ぬ ことで、 酸素などの 重い 元素が 増えていく 変化
ResearchResearch themes
初期宇宙に
*Illustrative image初期銀河の酸素量の多様性
JWSTの
*Illustrative image初期銀河の星形成とサイズ
JWSTの
*Illustrative image最遠方の原始銀河団の発見
GLASS-JWST
*Illustrative image再電離期の明るい銀河の探索
Superborg プロジェクトでは、
MembersFaculty
- Associate Professor森下 貴弘
VoicesStudent voices
Ratings and reviews reflect the experiences of individual current or former students, not the lab's official views. Whether a lab has reviews, or how many, says nothing about the lab itself.
Students who take part in an interview may receive a thank-you gift worth ¥1,000, regardless of what they say.
Student ratings (0 students)
--
--
--
--
--
--
Student voices answer questions like these
- What's great about this lab?
- What did you learn after joining?
- What's the vibe, and what is the professor like?
- Who is this lab for?
- Where do graduates go?
Your experience can help younger students choose their lab. Your name won't be shown.
Write a lab reviewAnonymous · Your draft is saved if you stopRelatedLabs similar to 森下 貴弘 研究室
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: “NASA-HS201427a-HubbleUltraDeepField” NASA, ESA, H. Teplitz and M. Rafelski (IPAC/Caltech), A. Koekemoer (STScI), R. Windhorst (Arizona State University), and Z. Levay (STScI) / Public domain (cropped)
- 初期銀河の
酸素量の 多様性: “The Phantom Galaxy Across the Spectrum” NASA's James Webb Space Telescope / CC BY 2.0 (cropped) - 初期銀河の
星形成と サイズ: “Most-Distant Galaxy Candidates in the Hubble Ultra Deep Field (opo0428b)” NASA, ESA, R. Windhorst (Arizona State University) and H. Yan (Spitzer Science Center, Caltech) / Public domain (cropped) - 最遠方の
原始銀河団の 発見: “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped) - 再電離期の
明る い 銀河の 探索: “Hubble 2009 close-up” NASA / Public domain (cropped) - Related lab (惑星大気物理学分野): “Mars atmosphere” NASA / Public domain (cropped)
- Related lab (富田 賢吾 研究室): “HD 163296 protoplanetary disk by ALMA (16CB25B)” ALMA (ESO/NAOJ/NRAO); A. Isella; B. Saxton (NRAO/AUI/NSF) / CC BY 4.0 (cropped)
- Related lab (村山 卓 研究室): “Messier83 - Heic1403a” Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA) Acknowledgement: William Blair (Johns Hopkins University) / Public domain (cropped)
- Related lab (海洋物理学分野): “Anton Dohrn am Liegeplatz in Bremerhaven” Manfred Stein / CC BY-SA 3.0 de (cropped)
About LabLog
LabLog is a lab review app for students only. Student members at each university interview students in labs and publish what they say. Student voices can only be read by students who sign up with a university email address. Operated by bestiee Inc.
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.