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2015-07

The double-ridge structure in high-frequency time-distance diagram / AGN Feedback toLow-mass Galaxy Formation at High Redshift / The Study of Large-scale Structure based on Wide – imaging observations using HSC

[Speaker1]
Nagaaki Kambara, M1, SOKENDAI, Mitaka(supervisor: SEKII Takashi , Watanabe, Tetsuya , Kubo Masahito)
[Title]
The double-ridge structure in high-frequency time-distance diagram

[Speaker2]
Satoshi Kikuta, M1, SOKENDAI, Mitaka(supervisor: Masatoshi Imanishi, Tadayuki Kodama, Yoshiki Matsuoka)
[Title]
AGN Feedback toLow-mass Galaxy Formation at High Redshift

[Speaker3]
Hisakazu Uchiyama, D1, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)
[Title]
The Study of Large-scale Structure based on Wide – imaging observations using HSC

How to Light Up the “Dark-Side” of the Universe? / Optical Seeing Properties on the Pointing Verification for ALMA Antenna / Detailed analyses of Lithium abundances in ultra metal-poor stars

[Speaker1]
Shogo Ishikawa, D2, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)
[Title]
How to Light Up the “Dark-Side” of the Universe?

[Speaker3]
Ayumu Matsuzawa, D3, SOKENDAI, Mitaka(supervisor: Satoru Iguchi)
[Title]
Optical Seeing Properties on the Pointing Verification for ALMA Antenna

[Speaker3]
Tadafumi Matsuno, M1, SOKENDAI, Mitaka(supervisor: Wako Aoki)
[Title]
Detailed analyses of Lithium abundances in ultra metal-poor stars

On the polarization in the solar atmosphere and how CLASP will measure it / Observation of the Inner Disk Region Around GG Tau A

[Speaker1]
GIONO Gabriel, D3, SOKENDAI, Mitaka (supervisor: Suematsu Yoshinori)
[Title]
On the polarization in the solar atmosphere and how CLASP will measure it
[Abstract]
Following some comments from my previous colloquium I think it is a good time to review in more details how the polarization is created by anisotropic illumination in the solar atmosphere and how the Hanle effect modifies this atomic polarization. I will also explain the measurement strategy behind our instrument (CLASP) and how it was calibrated to measure the Hanle effect of the Lyman-alpha line.

[Speaker2]
Sumire Tatehora, D3, SOKENDAI, Mitaka(supervisor : Nobuo Arimoto)

[Speaker3]
Yi Yang, D1, SOKENDAI, Mitaka (supervisor: Saeko Hayashi)
[Title]
Observation of the Inner Disk Region Around GG Tau A

Radiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow / The Wide-orbit Planetary Mass Companion Around Very Young Star with stellar-disk in early evolutionary stage / Weak Lensing Analysis of CL0016 Supercluster using Hyper Suprime‒Cam

[Speaker1]
Hiroshi Kobayashi, D2, SOKENDAI, Mitaka(supervisor: Ken Ohsuga)
[Title]
Radiation-MHD Simulation of Clumpy Outflow from Supercritical Accretion Flow

[Speaker2]
Daehyun Oh, D3, SOKENDAI, Mitaka(supervisor: Tamura Motohide)
[Title]
The Wide-orbit Planetary Mass Companion Around Very Young Star with stellar-disk in early evolutionary stage

[Speaker3]
Junya Sakurai ,D2, SOKENDAI, Mitaka(supervisor: Satoshi Miyazaki)
[Title]
Weak Lensing Analysis of CL0016 Supercluster using Hyper Suprime‒Cam

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