Program
The time is shown in JST (-1 hour in Taiwan) (That is, the program starts at 8:30 in Taiwan.)
| Thursday February 23, 2023 | |
|---|---|
| 10:00~10:45 | Chair: Kei Ito |
| 10:00~10:15 | Star formation history of mass selected galaxies at 0.1 < z < 1.5 in the ELAIS N1 Emmanuel Francis Ocran (Korea Astronomy and Space Science Institute) |
| 10:15~10:30 | SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Confusion-limited 450 μm Galaxy Number Counts and Machine Learning Identifications Zhen-Kai Gao (ASIAA/NCU) |
| 10:30~10:45 | Testing Lyman alpha emitters and Lyman-break galaxies as tracers of large-scale structures in the high-redshift universe. Sang Hyeok Im (Seoul National University) |
| 10:45~11:00 | Break |
| 11:00~11:45 | Chair: Kei Ito |
| 11:00~11:15 | Unknown Ionization Sources in Local Dwarf Galaxies Shun Hatano (SOKENDAI, NAOJ) |
| 11:15~11:30 | Mass-Metallicity Relation and Star Formation History of Dwarf Galaxies Explored by Galactic Archaeology Sena Matsui (Nagoya University) |
| 11:30~11:45 | Elucidating the role of interactions in galaxy evolution
Adarsh Ranjan (Korea Astronomy and Space Science Institute) |
| 11:45~13:30 | Lunch |
| 13:30~14:15 | Chair: Kei Ito |
| 13:30~13:45 | A distance ladder of cosmic ray feedback signatures in star-forming galaxies: the high-redshift domain Ellis Owen (Osaka University) |
| 13:45~14:00 | Emulating the 21cm global signal and analyzing the EDGES public data Shintaro Yoshiura (Mizusawa VLBI Observatory, NAOJ) |
| 14:00~14:15 | Tokult: A new code of galaxy kinematics taking gravitational lensing into account Yuma Sugahara (Waseda University / NAOJ) |
| 14:15~14:30 | Break |
| 14:30~15:30 | Chair: Taiki Kawamuro |
| 14:30~14:45 | Spatially resolved ISM properties and AGN-galaxy decomposition of HyLIRG at redshift 4.4 Takafumi Tsukui (Australian National University) |
| 14:45~15:00 | The average SMBH accretion properties of star-forming galaxies and their cosmic evolution over 4≲z≲7. Suin Matsui (The University of Tokyo) |
| 15:00~15:15 | Failed AGN feedback? -- Molecular reservoirs are not severely affected by extremely fast, kpc-scale AGN ionized-wind in ULIRGs at z~0.5 Xiaoyang Chen (NAOJ) |
| 15:15~15:30 | Hard X-ray to Radio Multiwavelength SED Analysis of Local U/LIRGs with Self-consistent AGN Model Including Polar-dust Component Satoshi Yamada (RIKEN) |
| 15:30~15:45 | Break |
| 15:45~16:30 | Chair: Taiki Kawamuro |
| 15:45~16:00 | Observational Evidence for Large-Scale Gas Heating in a Galaxy Protocluster at z=2.30 Chenze Dong (Kavli IPMU) |
| 16:00~16:15 | Environment of SDSS quasars at z = 0.3-1.0 traced by Subaru HSC Kohei Shibata (Ehime University) |
| 16:15~16:30 | High-resolution ALMA study of structure and gas kinematics of cluster galaxies at z =1.46 Ryota Ikeda (SOKENDAI/NAOJ) |
| 16:30~16:35 | CLOSING REMARKS |
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