コロキウム」カテゴリーアーカイブ

Opacity of fluffy dust aggregates / Status Overview of Space Gravitational-wave Detector Projects / Investigating the formation scenario of a massive star forming region IRAS18089-1732 from molecular line spectra

[Speaker1]
Akimasa Kataoka, D3, SOKENDAI, Mitaka(supervisor: Kohji Tomisaka)
[Title]
Opacity of fluffy dust aggregates

[Speaker2]
Koki OKUTOMI, M2, SOKENDAI, Mitaka(supervisor: Yoichi ASO, Raffaele FLAMINIO, Tomotada AKUTSU)
[Title]
Status Overview of Space Gravitational-wave Detector Projects

[Speaker3]
Nagisa Shino, D3, SOKENDAI, Mitaka(supervisor: Mareki Honma)
[Title]
Investigating the formation scenario of a massive star forming region IRAS18089-1732 from molecular line spectra

Measurement of Spin-Orbit Misalignment by Gravity Darkening Effect / Direct imaging for mid-mass giant having long term RV trend

[Speaker1]
Masahiro Onitsuka,D1, SOKENDAI, Mitaka(supervisor: Motohide Tamura)
[Title]
Measurement of Spin-Orbit Misalignment by Gravity Darkening Effect

[Speaker2]
Tsuguru Ryu,M2, SOKENDAI, Mitaka(supervisor: Saeko Hayashi)
[Title]
Direct imaging for mid-mass giant having long term RV trend

Inward motion of molecular gas in the center of NGC 1097 / Development of High-Accuracy Pointing Verification for ALMA Antenna

[Speaker1]
Kyoko Onishi, M3, SOKENDAI, Mitaka(supervisor: Satoru Iguchi)
[Title]
Inward motion of molecular gas in the center of NGC 1097

[Speaker2]
Ayumu Matsuzawa, M4, SOKENDAI, Mitaka(supervisor: Satoru Iguchi)
[Title]
Development of High-Accuracy Pointing Verification for ALMA Antenna

clustering properties of z~2 galaxies by extremely wide field galaxy survey etc.

[Speaker1]
Shogo Ishikawa , D1, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)
[Title]
clustering properties of z~2 galaxies by extremely wide field galaxy survey

[Speaker2]
Masafusa Onoue , M2, SOKENDAI, Mitaka(supervisor: Nobunari Kashikawa)
[Title]
The Selection Method for Finding High-z Quasar
[Abstract]
In this colloquium, I’d like to start with explaining how to estimate redshift of unknown objects, and why it is important. Then, I will show you the progress of the development of effective quasar selection method that I have been working on.