Chemical Network Simulations for Glycine Precursors / Observational study of the evolution of M BH / M spheroid ratios probed by z~3.3 QSOs

[Speaker 1]
Taiki Suzuki, D2, SOKENDAI, Mitaka(supervisor: Ohishi Maharishi)
[Title]
Chemical Network Simulations for Glycine Precursors

[Speaker 2]
Yuriko SAITO, D3, SOKENDAI, Mitaka(supervisor: Masatoshi Imanishi)
[Title]
Observational study of the evolution of M BH / M spheroid ratios probed by z~3.3 QSOs

総研大・国立天文台　スプリングスクール２０１５

３月９日（月）～１２日（木）までの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。５回目を迎えた今回は、全国２５大学から４１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、重力波天文学、光赤外線天文学、電波天文学、太陽物理学の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。

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What is the physical state of interstellar medium in high redshift galaxies? / The Extremely Wide-Field gzK Galaxy Survey / Speckle Nulling using SCExAO

[Speaker 1]
Rhythm Shimakawa ,D1, SOKENDAI, Mitaka(supervisor: Tadayuki Kodama)
[Title]
What is the physical state of interstellar medium in high redshift galaxies?
[Abstract]
I would like to review one of the most controversial issues in galaxy science, that is physical conditions of interstellar medium (ISM) in high redshift galaxies.
Many works seeking physical properties of star-forming galaxies at high redshifts have been published in recent years, and these are strongly suggesting that ISM conditions at high redshifts are different from those in the local Universe. This review will show
recent highlights of such kind of studies including our submitted letter (Shimakawa et al. arXiv:1411.1408).

[Speaker 2]
Shogo Ishikawa, D1, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)
[Title]
The Extremely Wide-Field gzK Galaxy Survey

[Speaker 3]
Prashant Pathak, D1, SOKENDAI, Mitaka(supervisor: Dr. Hideki Takami’)
[Title]
Speckle Nulling using SCExAO