Visit ASIAA Homepage Registration Deadline: November 1, 2018 (Taiwan Time)
East-Asia AGN Workshop 2019
January 21(Mon)-23(Wed), 2019
ASIAA Auditorium, 1st Floor AS/NTU Astronomy-Mathematics Building


Monday January 21, 2019
08:30~09:00 Registration
09:00~09:05 Welcome
09:05~09:10 Local Announcements
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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