Program

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Wednesday March 13, 2019
V: Multi-wavelength Studies of Clusters Chair: Changbom Park (KIAS)
09:00~09:20	Invited Halo Concentration, Galaxy Red Fraction, and Gas Properties of Optically-defined Merging Clusters Abstract Nobuhiro Okabe (Hiroshima Univ.)
09:20~09:40	Invited SZ Observations of HSC Clusters with MUSTANG2 Abstract Tony Mroczkowski (ESO)
09:40~09:55	X-ray observations of optically-selected galaxy clusters in the Subaru HSC-SSP field Abstract Naomi Ota (Nara Women's University)
09:55~10:10	Multi-wavelength Observations of Candidate Starbursting Protoclusters selected by Planck and Herschel Abstract Tai-An Cheng (Imperial College London)
10:10~10:30	Short Discussion IV
10:30~10:50	Coffee Break
VI: Future of Subaru: PFS+ULTIMATE Chair: Teppei Okumura (ASIAA)
10:50~11:10	Invited The current status of PFS project Abstract Kiyoto Yabe (Kavli IPMU)
11:10~11:30	Invited ULTIMATE-Subaru: toward the "bright" future of Subaru Telescope Abstract Yusei Koyama (Subaru Telescope)
11:30~11:45	Spectroscopic Identifications of Early Large Scale Structures with Protoclusters Over 200 Mpc Abstract Yuichi Harikane (The University of Tokyo)
11:45~12:00	Connection between star formation activities in galaxy clusters and surrounding environment Abstract Myungshin Im (Seoul National University)
12:00~12:15	Studying High-Redshift Protoclusters with IGM Tomography Abstract Khee-Gan Lee (Kavli IPMU)
12:15~12:30	The environmental impacts on the mass-metallicity relation at z=1.52. Abstract Shigeru Namiki (SOKENDAI, NAOJ)
12:30~13:30	Lunch
13:30~14:30	Discussion II: Cluster Studies with Subaru in the TMT/GMT era Chair: Taddy Kodama (Tohoku)
14:30~14:40	Concluding remarks Changbom Park (Korea Institute for Advanced Study)