児玉研究室@東北大天文教室
Kodama Labo @ Tohoku University

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 

Revealing the History of Galaxy and Cluster Formation and Evolution with Observations by Modern Telescopes (e.g., Subaru, ALMA, JWST) and Phenomenological Models

News

1 Apr 2024

【MEMBER】A graduate student (M1) and two B4 students have joined our team. info >>

1 Apr 2024

JSPS KAKENHI Specially Promoted Research "Towards Ultimate Subaru: Galaxy formation history probed by deep near-infrared imaging with wide-field adaptive optics" (PI: T. Kodama, FY2024-2030) has started.

TK is participating JSPS KAKENHI International Leading Research "Comprehensive understanding of the formation history of structures in the Universe" (PI: S. Miyazaki, 2022-2028).

Formation of galaxies and their clusters was most active around 100-120 Gyrs ago. We aim to see the galactic Universe across this peak epoch and obtain global and statistical views of galaxy formation and evolution (macroscopic approach) and at the same time spatially resolve the internal structures and kinematics within individual galaxies to understand the physical processes directly (microscopic approach). With the observational data obtained through modern telescopes and the phenomenological models to interpret them, we are revealing how the galaxies and clusters form and grow.
 
Macroscopic Approach : PISCES, MAHALO-Subaru, HSC-HSC, SWIMS-18, ULTIMATE-Subaru, etc.
Microscopic Approach : GRACIAS-ALMA, GANBA-Subaru, ALMA-3D, ULTIMATE-Subaru, etc.
Phenomenological Models : Spectral synthesis model, Chemical evolution, etc.

 

OUR PROJECTS

PISCES

Panoramic Imaging and Spectroscopy of Cluster Evolution with Subaru

MAHALO-Subaru

MApping HAlpha and Lines of Oxygen with Suabru 

GRACIAS-ALMA

Galaxy Resolved Anatomy with Co Interferometry And Submm observations with ALMA

HSC-HSC

Hybrid Search for Clusters with HSC

SWIMS-18

Superb Wide-field Imaging Multicolour Survey with 18 Filters on SWIMS

ALMA-3D

High resolution imaging and kinematics of galaxies at the cosmic noon 

GANBA-Subaru

Galaxy Anatomy with Narrow-Band Ao imaging with Subaru

ULTIMATE-Subaru

Ultra-wide Laser Tomographic Imager and MOS with AO for Transcendent Exploration

児玉 忠恭

Tadayuki Kodama
Professor

久保 真理子

Mariko Kubo
Assistant Professor

山本 直明

Naoaki Yamamoto
D3 student

大工原 一貴

Kazuki Daikuhara
D3 student

刘 兆然

Zhaoran Liu
D3 student

安達 孝太

Kota Adachi
D1 student

石田 光

Ko Ishida
M2 student

高橋 宏典

Kosuke Takahashi
M2 student

舩木 美空

Miku Funaki
M1 student
 
Ryo Sutanto
M1 student

萩原 颯

Hayate Hagiwara
B4 student

丸山 満ちる

Michiru Maruyama
B4 student
 

Major collobators

Masao Hayashi
Yusei Koyama, Subaru, Associate Prof.
Ken-ichi Tadaki, Hokkai Gakuen Univ., Associate Prof.
Rythm Shimakawa, Waseda Univ., Associate Prof.
Ichi Tanaka, Subaru, RCUH
Masato Onodera, Subaru, Assistant Prof.
Yosuke Minowa, Subaru, Associate Prof.
Jun Toshikawa,Nishiharima Obs., Staff
Minju Lee, Dawn, Postdoc fellow
Kentaro Motohara, Univ. of Tokyo/NAOJ, Professor
Masahiro Konishi, Univ. of Tokyo, Assistant Professor
José Manuel Perez Martinez,  IAC, Marcury fellow
Haruka Kusakabe, NAOJ, JSPS PD fellow
Takahiro Morishita, Caltech/IPAC, Staff scientist
Zhiying Mao, Padova, Postdoc fellow
Ronaldo Laishram, NAOJ, Postdoc fellow

OB/OG

Tomoko Suzuki
Moegi Yamamoto
Daiki Kimura
Nao Fukagawa
Kohei Aoyama
Masaharu Tamura
Zhiying Mao
Ronaldo Laishram
Riho Okazaki

Tadayuki Kodama (Dr./Prof.)
(Rm. S511, Science Complex C)
Astronomical Institute, Tohoku University
6-3 Aramaki, Aoba-ku, Sendai 980-8578
 
E-mail: kodama_at_astr.tohoku.ac.jp
Tel: 022-795-6503, Fax: 022-795-6513