「コロキウム」カテゴリーアーカイブ

Deep NIR spectroscopy for [OIII] emission line galaxies at z>3 / The accelerated build-up of the red sequence in high-redshift galaxy clusters (The review of Cerulo+16)

[Speaker 1]
Tomoko Suzuki, D3, SOKENDAI (Supervisor; Tadayuki Kodama)
[Title]
Deep NIR spectroscopy for [OIII] emission line galaxies at z>3
[Abstract]
I will show our preliminary results obtained by recent near-infrared spectroscopy for narrow-band-selected star-forming galaxies at z>3 with Keck/MOSFIRE.

[Speaker 2]
Moegi Yamamoto, D1, SOKENDAI (Supervisor; Tadayuki Kodama)
[Title]
The accelerated build-up of the red sequence in high-redshift galaxy clusters (The review of Cerulo+16)

Formation Path of Interstellar Glycine / Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) / A Search for the Cause of Low Lithium Abundances in Some Extremely Metal-Poor Stars

[Speaker1]
Taiki Suzuki, D3, SOKENDAI (Supervisor: Masatoshi Ohishi)
[Title]
Formation Path of Interstellar Glycine

[Speaker2]
Masafusa Onoue, D2, SOKENDAI (Supervisor: Nobunari Kashikawa)
[Title]
Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs)
[Abstract]
I will present recent updates of high-redshift (z>6) quasar search project using Hyper Suprime-Cam Subaru Strategic Program (HSC-SSP) survey, with which we have succeeded in identifying 9 z>6 quasars from the initial data release. Also, I will show the result of another faint quasar search at z~6 using deep Subaru/Suprime-Cam images.

[Speaker3]
Tadafumi Matsuno, M2, SOKENDAI (Supervisor: Wako Aoki)
[Title]
A Search for the Cause of Low Lithium Abundances in Some Extremely Metal-Poor Stars

Science cases based on narrow-band data with HSC-SSP / AGN feedback to neighbouring galaxy formation

[Speaker 1]
Rhythm Shimakawa, D3, SOKENDAI (supervisor : Tadayuki Kodama)
[Title]
Science cases based on narrow-band data with HSC-SSP
[abstract]
In this talk, I will describe how to find distant galaxies up to z~1.7 by capturing the unique spectral features by narrow-band filters based on the HSC-SSP data. I will then present some actual examples of narrow-band selected galaxies (Hα, [OIII], [OII] emitters) and Balmer break galaxies at 0.4

Direct imaging observations of intermediate mass giants with RV trends II / Correlation between protoclusters and QSOs using HSC

[Speaker1]
Tsuguru Ryu, D2, SOKENDAI (supervisor : Saeko Hayashi)
[Title]
Direct imaging observations of intermediate mass giants with RV trends II

[Speaker2]
Hisakazu Uchiyama, D2, SOKENDAI, Mitaka（supervisor : Nobunari Kashikawa）
[Title]
Correlation between protoclusters and QSOs using HSC