座長団 (Chairpersons)
上から順に、名前、所属、勉強・研究分野、webpage
from top to buttom, name, affiliation, reserch activity and webpage
池田浩之 (Hiroyuki Ikeda)
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愛媛大学 数理物質科学専攻 D1
1st year Ph.D course, Department of Mathematics, Physics, and Earth Sciences,
Ehime University.
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広域サーベイによる超巨大ブラックホールの進化の観測的研究
Observational Studies of the evolution of supermassive BH
by wide-field surveys
服部公平 (Kohei Hattori)
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東京大学 天文学教育研究センター D1
1st year Ph.D course, Institiute of Astronomy, University of Tokyo.
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銀河系のハロー星の運動解析に基づく銀河系形成史の解明
Studies on kinematics of the Milky Way halo stars
by analitic modeling
林隆之 (Takayuki Hayashi)
- 東京大学 天文学専攻 / 国立天文台 水沢VLBI観測所 D1
1st year Ph.D course, Astronomical Institute, University of Tokyo
/ NAOJ VLBI Observatory.
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電波干渉計と光赤外高分散分光による
電波ジェットと活動銀河核アウトフローの共進化に対する観測的研究
Observational studies of co-evolution between radio jets and AGN outflow
with radio interferometers and high-dispersion spectroscopy at rest-UV
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webpage
市川幸平 (Kohei Ichikawa)
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京都大学 宇宙物理学教室 M2
2nd year Master course student, Department of Astronomy Kyoto University.
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赤外線/X線を用いての(U)LIRGを含めた隠されたAGNの成長に対する観測的研究
Observational studies of obscured AGNs and (U)LIRG with infrared and X-ray.
中村翔 (Sho Nakamura)
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東北大学 天文学専攻 M2
2nd year Master course, Astronomical Institute Tohoku University.
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磁気流体シミュレーションによる銀河円盤モデル構築
Galaxy disc modeling by MHD simulation
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webpage
1st year Ph.D course, Department of Mathematics, Physics, and Earth Sciences, Ehime University.
Observational Studies of the evolution of supermassive BH by wide-field surveys
1st year Ph.D course, Institiute of Astronomy, University of Tokyo.
Studies on kinematics of the Milky Way halo stars by analitic modeling
1st year Ph.D course, Astronomical Institute, University of Tokyo / NAOJ VLBI Observatory.
Observational studies of co-evolution between radio jets and AGN outflow with radio interferometers and high-dispersion spectroscopy at rest-UV
2nd year Master course student, Department of Astronomy Kyoto University.
Observational studies of obscured AGNs and (U)LIRG with infrared and X-ray.
2nd year Master course, Astronomical Institute Tohoku University.
Galaxy disc modeling by MHD simulation