Program
Monday March 11, 2019 | |
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08:30~08:50 | Registration |
08:50~09:00 | Announcement LOC |
I: HSC & Sister Cluster Surveys Chair: Yen-Ting Lin (ASIAA) |
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09:00~09:30 | Invited Shear selected clusters catalogs based on HSC-SSP Satoshi Miyazaki (National Astronomical Observatory of Japan) |
09:30~09:50 | Invited HSC data release Sogo Mineo (NAOJ) |
09:50~10:10 | Invited An optically selected HSC cluster catalog Masamune Oguri (University of Tokyo) |
10:10~10:30 | Invited Galaxy quenching explored with HSC^2, PFS^2, and ULTIMATE-K Tadayuki Kodama (Tohoku University) |
10:30~10:50 | Coffee Break |
10:50~11:10 | Invited A systematic search for protoclusters based on Subaru/HSC survey Jun Toshikawa (University of Tokyo) |
11:10~11:25 | Hyper Suprime-Cam Weak Lensing Measurement of Galaxy Clusters selected by Atacama Cosmology Telescope Hironao Miyatake (Nagoya University) |
11:25~11:40 | HectoMAP Galaxy Cluster Surveys Jubee Sohn (Havard-Smithsonian Center for Astrophysics) |
11:40~11:55 | Probing large-scale structures with emission-line galaxies selected from HSC narrow-band data Masao Hayashi (National Astronomical Observatory of Japan) |
11:55~12:15 | Short Discussion I |
12:15~13:30 | Lunch |
II: Cluster Galaxy Population Chair: Masao Hayashi (NAOJ) |
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13:30~13:50 | Invited Stripping, quenching and morphological transformations of cluster galaxies according to the IllustrisTNG simulations Annalisa Pillepich (MPIA Heidelberg) |
13:50~14:10 | Invited How fast is the evolution of galaxies in clusters? Benedetta Vulcani (INAF - OaPD) |
14:10~14:25 | Star formation in cluster galaxies since z~1 Howard Yee (University of Toronto) |
14:25~14:40 | Exploring cluster galaxy evolution with the HSC survey Yen-Ting Lin (ASIAA) |
14:40~14:55 | The brightest UV-selected galaxies in protoclusters at z~4: Ancestors of Brightest Cluster Galaxies? Kei Ito (SOKENDAI/NAOJ) |
14:55~15:25 | Coffee Break |
15:25~15:45 | Invited Galaxy populations in the most distant SPT-SZ clusters: the evolution of galaxies in the first massive cluster environments Veronica Strazzullo (Ludwig-Maximilians-Universität München) |
15:45~16:00 | Why are the galaxies in clusters gas poor? Lessons from simulations Sukyoung Yi (Yonsei University) |
16:00~16:15 | Unveiling Quenching History of Cluster Galaxies Using Phase-space Analysis Jinsu Rhee (Yonsei Univ.) |
16:15~16:30 | The kinematic morphology - density relationship in clusters Sarah Brough (University of New South Wales) |
16:30~16:45 | Modelling galaxy quenching and spatial distributions of star-forming and quenched galaxies Taira Oogi (Kavli IPMU) |
16:45~17:10 | Short Discussion II |