Program
| Monday January 21, 2019 | |
|---|---|
| 08:30~09:00 | Registration |
| 09:00~09:05 | Welcome SOC |
| 09:05~09:10 | Local Announcements LOC |
| 09:10~09:35 | Invited China's Telescope Access Program(TAP): the past, present, and future Y.Sophia Dai (NAOC) |
| 09:35~09:55 | A Direct Test of AGN Feedback Luis Ho (Kavli Institute for Astronomy and Astrophysics, Peking University) |
| 09:55~10:15 | The Star Formation Efficiency of Quasar Host Galaxies at Low Redshifts Yanxia Xie (The Kavli Institute for Astronomy and Astrophysics at Peking University) |
| 10:15~10:35 | Co-evolution of AGN and bulges: AGN are more common in real bulges than in pseudobulges Hassen Yesuf (Kavli PKU/ Kavli IMPU) |
| 10:35~11:15 | Group Photo / Poster session (and coffee break) |
| 11:15~11:40 | Invited Korean 8m Class Optical Facility: Gemini Observatory Narae Hwang (KASI) |
| 11:40~12:00 | Ionized gas outflows in z~2 WISE-selected Hot Dust Obscured Galaxies Hyunsung Jun (Korea Institute for Advanced Study) |
| 12:00~12:20 | Dynamical modeling of AGN outflows with seeing effect using Type 2 AGNs Jaejin Shin (Seoul National University) |
| 12:20~12:45 | Invited Current Status of the Subaru Telescope and its future prospect Nagayoshi Ohashi (Subaru Telescope) |
| 12:45~14:15 | Lunch |
| 14:15~14:35 | Structures of AGN Host Galaxies Yu-Yen Chang (ASIAA) |
| 14:35~14:55 | Investigating the connection between AGNs and their host galaxy properties Li-Ting Hsu (ASIAA) |
| 14:55~15:25 | Discussion1: AGN Host Galaxies, Co-evolution, Feedback, Feeding |
| 15:25~15:45 | Coffee Break |
| 15:45~16:05 | Imaging the interstellar medium in the most distance quasar host galaxies Ran Wang (Kavli institute for astronomy and astrophysics, Peking University) |
| 16:05~16:25 | Discovery of a z = 4.7 Radio Galaxy without an Ultra-steep Spectrum Takuji Yamashita (Ehime University) |
| 16:25~16:45 | One step toward understanding cosmic re-ionization: absorption tests with a new QSO we discovered at z=6.6 Tomo Goto (NTHU) |
| 16:45~17:05 | Does AGN Fraction Have Redshift or Luminosity Dependence? An Extinction-Free Test based on the 18-bands Infrared SED Fitting using AKARI NEP Wide Data Seong-Jin Kim (NTHU) |
| 17:05~17:35 | Discussion2: High-z AGNs |
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