GALAXY EVOLUTION WORKSHOP 2021
GALAXY EVOLUTION WORKSHOP 2021
February 7(Mon)-10(Thu), 2022
Online

Program

The time is shown in JST (-1 hour in Taiwan) (That is, the program starts at 9:00 in Taiwan.)

Thursday February 10, 2022
10:00~10:15 The global structure of the Milky Way's stellar halo based on the orbits of local metal-poor stars
Genta Sato (Tohoku University)
10:15~10:30 Stellar population and motion in the Galactic halo substructure using HSC and Gaia data
Yoshihisa Suzuki (Astronomical Institute, Tohoku University)
10:30~10:45 Statistical Verification of the Missing Satellites Problem outside the Local Group
Masashi Nashimoto (NAOJ)
10:45~11:00 Dark Matter Deficient Galaxies and Their Member Star Clusters Form Simultaneously during High-velocity Galaxy Collisions in 1.25 pc Resolution Simulations
Joohyun Lee (University of Texas at Austin)
11:00~11:15 Break
11:15~11:30 Properties of Fast and Slow Bars Classified by Epicyclic Frequency Curves from Photometry of Barred Galaxies
Yun Hee Lee (Korea Astronomy and Space Science Institute (KASI))
11:30~11:45 CO(2–1)/CO(1–0) line ratio on a ∼100 parsec scale in the nearby barred galaxy NGC 1300
Fumiya Maeda (Univ. of Tokyo)
11:45~12:00 Analysis of the spatially resolved SFR – M relation for DustPedia galaxies
Wen SHI (Nagoya University)
12:00~12:15 Spatially Resolved Panchromatic SED fitting of Nearby Galaxies: Resolved Properties of Stars, Dust, and Gas
Abdurro'uf Abdurro'uf (ASIAA)
12:15~12:30 GalWeight-Derived SDSS Galaxy Cluster Catalog and Cosmological Constraints on the omega_m and sigma_8
Mohamed Elhashash (Institute of Management and Information Technologies, Chiba University)
12:30~14:00 Lunch Break
14:00~14:15 Developing new recipes for measuring the dynamical state of galaxy clusters using simulations.
Hyowon Kim (UST/KASI)
14:15~14:30 How to quantify the similarity of 2D distributions: Comparison of spatial distribution of Intracluster light and Dark Matter
Jaewon Yoo (KASI/UST)
14:30~14:45 Mass-Velocity Dispersion Relation on MaNGA Brightest Cluster Galaxies
Yong Tian (National Central University)
14:45~15:00 A systematic search for galaxy protocluster cores at the transition epoch of their star formation activity
Makoto Ando (The University of Tokyo)
15:00~15:15 Star formation and chemical evolution in protocluster
Keita Fukushima (Osaka University)
15:15~15:30 Gas-phase environmental effects in the Spiderweb protocluster at z=2.16
Jose Manuel Perez-Martinez (Tohoku University)
15:30~15:40 Break
15:40~15:55 The same and not the same: Different star formation properties of high redshift galaxy clusters
Seong-Kook Lee (Seoul National University)
15:55~16:10 Growth of the brightest cluster galaxy NGC 1275 in the cool-core Perseus cluster
Youichi Ohyama (ASIAA)
16:10~16:25 Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
Jaehyun Lee (Korea Institute of Advanced Study)
16:25~16:45 Poster & Break
16:45~17:00 An ACA CO survey of the IC 1459 group and the NGC 4636 group: environmental effects on molecular gas of group galaxies
Bumhyun Lee (Korea Astronomy and Space Science Institute)
17:00~17:15 Search for fading AGNs at z < 0.4
Janek Pflugradt (Tohoku University)
17:15~17:30 Testing Web Feeding Model for Star Formation in Galaxy Clusters in the COSMOS Field
Eunhee Ko (Seoul National University)
17:30 CLOSING REMARK
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