Formation of galaxies and their clusters was most active around 100-120 Gyrs ago. We aim to see the galactic Universe across this peak epoch and obtain global and statistical views of galaxy formatino and evolution (macroscopic approach) and at the same time spatially resolve the internal structures and kinematics within individual galaxies to understand the physical processes directly (microscopic approach). With the observational data obtained through modern telescopes and the phenomenological models to interpret them, we are revealing how the galaxies and clusters form and grow.
Macroscopic Approach : PISCES, MAHALO-Subaru, HSC-HSC, SWIMS-18, ULTIMATE-Subaru, etc.
Microscopic Approach : GRACIAS-ALMA, GANBA-Subaru, ALMA-3D, ULTIMATE-Subaru, etc.
Phenomenological Models : Spectral synthesis model, Chemical evolution, etc.
PISCES
Panoramic Imaging and Spectroscopy of Cluster Evolution with Subaru
MAHALO-Subaru
MApping HAlpha and Lines of Oxygen with Suabru
GRACIAS-ALMA
Galaxy Resolved Anatomy with Co Interferometry And Submm observations with ALMA
HSC-HSC
Hybrid Search for Clusters with HSC
SWIMS-18
Superb Wide-field Imaging Multicolour Survey with 18 Filters on SWIMS
ALMA-3D
High resolution imaging and kinematics of galaxies at the cosmic noon
GANBA-Subaru
Galaxy Anatomy with Narrow-Band Ao imaging with Subaru
ULTIMATE-Subaru