9th GALAXY EVOLUTION WORKSHOP
9th GALAXY EVOLUTION WORKSHOP
February 20(Mon)-23(Thu), 2023
Kyoto University Science Seminar House

Program

The time is shown in JST (-1 hour in Taiwan) (That is, the program starts at 8:30 in Taiwan.)

Monday February 20, 2023
09:30~09:35 OPENING
09:35~10:50 Chair: Takuma Izumi
09:35~10:05 Invited JWST: Early History and Early Results on Galaxy Evolution
Myungshin Im (Seoul National University)
10:05~10:20 Resolved dust emission of typical star-forming galaxies at z=4-6
Ikki Mitsuhashi (University of Tokyo)
10:20~10:35 Ruby-Rush: The quest of red monsters lurking in the protoclusters at z~5.
Kosuke Takahashi (Tohoku University)
10:35~10:50 JWST catches the mass assembly of z~5 ultra-low-mass galaxies
Yoshihisa Asada (Kyoto Univ.)
10:50~11:05 Break
11:05~12:15 Chair: Takuma Izumi
11:05~11:20 The Milky Way Tomography with Subaru Hyper Suprime-Cam. I. Halo substructures
Yoshihisa Suzuki (Astronomical Institute, Tohoku University)
11:20~11:35 First JWST results of local luminous infrared galaxies from GOALS
Hanae Inami (Hiroshima University)
11:35~11:50 Effects of non-circular motions in galaxies: from low-resolution IFS-galaxy surveys to high-spatial-resolution.
Carlos Lopez-coba (ASIAA)
11:50~12:05 Spin Catalog of Galaxies - Search for Symmetry Breaking in the distribution of galaxy spin vector
Masanori Iye (NAOJ(Prof.Emeritus), Japan Academy)
12:05~12:20 FLASH TALKS (1 min x 9 persons)
12:20~13:45 Lunch
13:45~15:00 Chair: Kohei Hayashi
13:45~14:15 Invited Stellar morphology of dusty star-forming galaxies at cosmic noon
Chian-Chou Chen (tc) (ASIAA)
14:15~14:30 Colder and Dustier! Probing Dust Properties of the Brightest Submillimeter Galaxies at Cosmic Noon
Cheng-Lin Liao (NTU/ASIAA)
14:30~14:45 Galaxy quenching at high redshift revealed with multiwavelength observation
Tomoko Suzuki (Kavli IPMU)
14:45~15:00 The Growth of Far-IR Galaxies and Their Central Supermassive Black Holes at Intermediate Redshift
Kota Sakuma (Tohoku University)
15:00~15:15 Break
15:15~16:30 Chair: Yoshiki Toba
15:15~15:45 Invited JWST mid-infrared number counts and inferred cosmic star-formation history
Tomo Goto (National Tsing Hua University)
15:45~16:00 Black Hole and Galaxy Coevolution in X-Ray Selected Type-1 Quasars at 0.2
Kenta Setoguchi (Kyoto University)
16:00~16:15 Radiative transfer calculations for dense molecular gas based on the radiation-driven fountain model
Shunsuke Baba (鹿児島大学)
16:15~16:30 Circumnuclear multi-phase gas around the central AGN in a cool-core cluster, A1644-South
Junhyun Baek (Yonsei University)
16:30~16:45 Break
16:45~17:45 Chair: Daichi Kashino
16:45~17:00 Leaving no branches behind: An accurate model for predicting galaxy properties from full sets of merger trees of host dark matter halos
Chen-Yu Chuang (ASIAA/NTHU)
17:00~17:15 Machine learning based approach for merger classification in HSC-SSP and quantitative investigations on role of environment in merger activity
Kiyoaki Christopher Omori (Nagoya University)
17:15~17:30 Fitting Simulated Galaxies to Observations
Suchetha Cooray (Nagoya University)
17:30~17:45 Statistical study of RQGs in preparation for Subaru/PFS survey
Zhiying Mao (Tohoku University)
POSTER FLASH TALKS
Day1 Monday, 20 Feb 2023, 12:05–12:20
12:05 Rogerio Monteiro-Oliveira Is the dichotomy among early-type galaxies real? (via zoom)
Abstract
  Jeeun Hwang Constructing GALEX UV Catalog of Nearby Galaxies (via zoom)
Abstract
  Yoshiki Toba How do galaxy mergers affect the ionized gas kinematics of galaxies? ~KOOLS-IFU/Seimei view of local U/LIRGs~
Abstract
  Kei Ito Discovery of a protocluster of massive quiescent galaxies at z = 2.77
Abstract
  Aika Oki Elucidating co-evolutions among AGN, galaxies, and ICM from an AGN survey with VERA
Abstract
  YUYA NAKATANI Nuclear Structure in Radio Galaxies by Broadband X-Ray Spectral Analysis
Abstract
  Yuri Oku Cosmological hydrodynamical simulation for the galaxy-IGM study in the PFS era
Abstract
  Naoki Matsumoto MIR Search of Heavily Obscured z > 3 AGN Missed in X-ray Surveys
Abstract
12:20 Yongjung Kim IMS High-z Quasar Survey and Future
Abstract
ASIAA will not contact participants for credit card information. Privacy and Security Policy