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Panchromatic Panoramic Studies of Galaxy Clusters: from HSC to PFS and ULTIMATE
March 11(Mon)-13(Wed), 2019
ASIAA, Taipei, Taiwan

Invited Presentation

Galaxy quenching explored with HSC^2, PFS^2, and ULTIMATE-K

Author(s): Tadayuki Kodama (Tohoku) and HSC^2 team

Presenter: Tadayuki Kodama (Tohoku University)

We are conducting a project on distant clusters named Hybrid Search
for Clusters with HSC (HSC^2). This provides excellent opportunities
for us to investigate galaxy quenching (mass and environment) with
hundreds of galaxy clusters and post-starburst galaxies therein at
0.4 survey named Panoramic Follow-up Survey with PFS (PFS^2), which aims
to resolve recent star formation and quenching histories of individual
galaxies by placing constraints on timescale and burstiness. We are
also planning to expand such systematic cluster survey back in time to
z~5 with wide-field NIR (in particular K-band) imaging survey with
ULTIMATE-Subaru, using lots of narrow- and medium-band filters.

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