The current understanding of the stellar differential rotation / Doppler Tomographic Measurement for Orbital Precession of WASP-33b

[Speaker1]
Yoshiki Hatta, SOKENDAI: D1 (Supervisor : Takashi Sekii , Tetsuya Watanabe, Yukio Katsukawa)
[Title]
The current understanding of the stellar differential rotation

[Speaker2]
Noriharu Watanabe, SOKENDAI: D1 (Supervisor : Motohide Usuda, Norio Narita)
[Title]
Doppler Tomographic Measurement for Orbital Precession of WASP-33b

Detecting proto-BCG candidates at z~4 by using HSC-SSP / Gas inflow and outflow of star forming galaxies at redshift 1.4 as revealed by chemical evolution

[Speaker1]
Kei Ito, SOKENDAI 2nd year (M2)(Supervisor: Nobunari Kashikawa,Yuichi Matsuda,Yusei Koyama)
[Title]
Detecting proto-BCG candidates at z~4 by using HSC-SSP

[Speaker2]
Nao Fukagawa, SOKENDAI 3rd year (D1)(Supervisor: Prof. Tadayuki Kodama,,)
[Title]
Gas inflow and outflow of star forming galaxies at redshift 1.4 as revealed by chemical evolution
[Abstract]
Gas inflow and outflow are processes that control star formation history of galaxies. Using chemical evolution models, we attempt to extract information about gas inflow and outflow of star forming galaxies at redshift z~1.4. In this talk, we discuss our results.

総研大・国立天文台 スプリングスクール2018

 2月26日(月)~3月1日(木)の4日間、国立天文台三鷹キャンパスで、総研大・国立天文台スプリングスクールが開校されました。平成23年から始まったスプリングスクール。8回目を迎えた今回は、北は北海道から南は沖縄まで全国31大学から59名の参加者が集まりました。

最先端の研究者を講師陣として、理論天文学、電波天文学、光赤外線天文学、太陽物理学、装置開発の5つの天文学講義を4日間にわたって受講していただきました。また、今回は新企画として、参加者を8つの班に分けた体験学習も行いました。

続きを読む

A start to understand the relation between galaxies and IGM in the most over-dense regions / Exploration of the Cosmic Dawn with High-Redshift Quasars / Detecting Brightest Cluster Galaxies at z~4 by using Hyper Suprime-Cam

[Speaker 1]
Liang, Yongming, SOKENDAI 1st year (M1)(Supervisor: Kashikawa, Nobunari,,)
[Title]
A start to understand the relation between galaxies and IGM in the most over-dense regions

[Speaker 2]
Masafusa Onoue, SOKENDAI 5th year (D3)(Supervisor: Nobunari Kashikawa,,)
[Title]
Exploration of the Cosmic Dawn with High-Redshift Quasars

[Speaker 3]
Kei Ito, SOKENDAI 1st year (M1)(Supervisor: Nobunari Kashikawa,Yuichi Matsuda,Yusei Koyama)
[Title]
Detecting Brightest Cluster Galaxies at z~4 by using Hyper Suprime-Cam