Program

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

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Wednesday February 22, 2023
09:30~10:30	Chair: Ho Seong Hwang
09:30~09:45	ALMA Lensing Cluster Survey: Physical properties of intrinsically faint near-infrared dark galaxies at z~3-4 Abstract Akiyoshi Tsujita (The University of Tokyo)
09:45~10:00	Spectroscopic observation of massive quenching galaxy at z=4.53. Abstract Takumi Kakimoto (The Graduate University for Advanced Studies (SOKENDAI))
10:00~10:15	Properties of low-mass Hα emitters at z ∼ 2.3 from broad-band selection in the ZFOURGE Survey Abstract Nuo Chen (The University of Tokyo)
10:15~10:30	ALMA Lensing Cluster Survey: Full SED Analysis of Distant Galaxies Detected by Millimeter Observation Abstract Ryosuke Uematsu (Kyoto University)
10:30~10:45	Break
10:45~12:00	Chair: Kohei Hayashi
10:45~11:00	Understanding the cause of diverse rotation curves of nearby galaxies with cosmological hydrodynamical simulations Abstract Daeun Jeong (Seoul National University)
11:00~11:15	The Nascence of Disk Galaxies : Angular Momentum and its Impact on the Mass-Size Relation” Abstract Ji Hoon Kim (Astronomy Research Center, Seoul National University)
11:15~11:30	Kinematics of galaxies with early star formation explored by IFU observations of local Extremely Metal-Poor Galaxies Abstract Yi Xu (University of Tokyo)
11:30~11:45	Unveiling the Nature of Dark Galaxies with the IllustrisTNG Simulation Abstract Gain Lee (Seoul National University)
11:45~12:00	Star formation variability as a probe for the baryon cycle within galaxies Abstract Eun-jin Shin (Seoul National University)
12:00~13:30	Lunch
13:30~15:00	Chair: Yoshiki Toba
13:30~14:00	Invited First Results of High-redshift Low-Luminosity Quasar Studies with JWST Abstract Masafusa Onoue (Peking University KIAA / Kavli IPMU)
14:00~14:15	Finding of 29 radio-loud dust obscured galaxies: Are they super-Eddington candidates? Abstract Hikaru Fukuchi (Tohoku University)
14:15~14:30	The dark halo mass of quasars at z~6 with SHELLQs Abstract Junya Arita (The University of Tokyo)
14:30~14:45	Discovery of a Tight Correlation between Mm-wave and X-ray emission for Hard X-ray Selected Nearby AGNs Abstract Taiki Kawamuro (RIKEN)
14:45~15:00	X-ray Radiatively-driven extremely-fast clumpy outflow in the superEddington AGN Abstract Misaki Mizumoto (Kyoto University)
15:00~15:15	Break
15:15~16:30	Chair: Ho Seong Hwang
15:15~15:30	Clusters of Massive Quiescent Galaxies at z>2 Abstract Tomokazu Kiyota (Kyoto University)
15:30~15:45	Mining for the Protoclusters at z〜4 from HSC-SSP photometric dataset with Deep Learning Abstract Yoshihiro Takeda (The University of Tokyo)
15:45~16:00	Enhanced star-forming activity in a young proto-cluster at the cosmic noon probed by deep narrow-band imgaing Abstract Kazuki Daikuhara (Tohoku University)
16:00~16:15	Spatial Distribution Study of Intracluster Light vs. Dark Matter using HR5 Abstract Jaewon Yoo (Korea Institute for Advanced Study)
16:15~16:30	Evolutionary Stages of Galaxy Cluster in the Distant Universe: Younger Galaxy Cluster Candidates at z~1.5 Abstract Naoaki Yamamoto (Tohoku University)
16:30~16:45	Break
16:45~17:45	Chair: Daichi Kashino
16:45~17:00	A comprehensive report of the MAMMOTH-Subaru survey detecting LAEs and LABs traced by IGM/AGN at Cosmic Noon Abstract Yongming Liang (University of Tokyo/ICRR)
17:00~17:15	Constraining the distribution of cosmic baryons from FLIMFLAM survey Abstract Khrykin Ilya (Kavli IPMU)
17:15~17:30	Subhalo abundance matching with progenitor mass at varying redshift: Emergence of the ex-/in-situ stellar mass growth in HSC galaxy clustering? Abstract Shogo Masaki (National Institute of Technology, Suzuka College)
17:30~17:45	Exploring the coevolution of two dynamically distinct protoclusters and their galaxy populations at the cosmic noon Abstract Jose Manuel Perez-martinez (Tohoku University)