投稿者「guas-writer」のアーカイブ

Study of High-Energy Phenomena in the Solar Corona Tackled with X-ray Imaging-Spectroscopy / Spectroscopic study of the source region for fast Solar Wind acceleration in CH

[Speaker1]
Yoshiaki Sato
SOKENDAI 1st year (M1)
(Supervisor: Takashi Sekii,  Noriyuki Narukage, Masumi Simojo)
[Title1]
Study of High-Energy Phenomena in the Solar Corona Tackled with X-ray Imaging-Spectroscopy

[Speaker2]
Yoshihiro Naito
SOKENDAI 1st year (M1)
(Supervisor: Hirohisa Hara,  Ryoko Ishikawa, Joten Okamoto)
[Title2]
Spectroscopic study of the source region for fast Solar Wind acceleration in CH

The Origin of Rich Iron in Extremely Metal-poor Galaxies Probed by Core Collapse Supernova Model / Development of high precision detector calibration methods for astrometry and precision photometry with JASMINE / Light curves of electron capture and low mass Fe core collapse supernovae

[Speaker1]
Kuria Watanabe
SOKENDAI 1st year (M1)
(Supervisor: Masami Ouchi,  Nozomu Tominaga, Masato Onodera)
[Title1]
The Origin of Rich Iron in Extremely Metal-poor Galaxies Probed by Core Collapse Supernova Model

[Speaker2]
Shotaro Tada
SOKENDAI 3rd year (D1)
(Supervisor: Takayuki Kotani,  Yutaka Hayano, Yosuke Minowa)
[Title2]
Development of high precision detector calibration methods for astrometry and precision photometry with JASMINE

[Speaker3]
Masato Sato
SOKENDAI 3rd year (D1)
(Supervisor: Nozomu Tominaga,  Tomoya Takiwaki, Takashi Moriya)
[Title3]
Light curves of electron capture and low mass Fe core collapse supernovae

 

GRB REDSHIFT CLASSIFICATION USING MACHINE LEARNING / Unknown Ionization Sources in Extremely Metal Poor Galaxies.+ The Ionizing Spectrum of a z=7.67 Galaxy Observed by JWST.

[Speaker1]
Shubham Bhardwaj
SOKENDAI 3rd year (D1)
(Supervisor: Dainotti, Maria Giovanna, Nozomu Tominaga, Kazunari Iwasaki)
[Title1]
GRB REDSHIFT CLASSIFICATION USING MACHINE LEARNING

[Speaker2]
Shun Hatano
SOKENDAI 1st year (M1)
(Supervisor: Masami Ouchi,  Yusei Koyama, Takashi Moriya)
[Title2]
Unknown Ionization Sources in Extremely Metal Poor Galaxies.+ The Ionizing Spectrum of a z=7.67 Galaxy Observed by JWST.