Cosmology and High-energy Astrophysics
This key science is to study Cosmic Microwave Background (CMB) and large-scale structure in the Universe to understand the origin, composition and evolution of the universe. This study also includes searching and studying of pulsar, Fast Radio Burst (FRB) as well as dark matter and dark energy. Lastly, multi-messengers are used to investigate Active Galactic Nuclei (AGN), mass increment of supermassive black hole.
Research Study Guideline
Extragalactic astronomy
Extragalactic observations using the JWST
SEA OtTeRS: Synergy in Extragalactic Astronomy with Observation through Temporal and Redshift Spaces (with TNT and GTC)
Multi-messenger
Multi-messengers are used to investigate core-collapse supernovae, Active Galactic Nuclei (AGN), mass increment of supermassive black holes.
Jiangmen Underground Neutrino Observatory (JUNO) and Cherenkov Telescope Array (CTA)
POLARBEAR: Cosmic microwave background polarization experiment
Develope instrumentation: CoLoRS, DARTS and Freeform Optics Technology
Gravitational Wave
Gravitational wave optical transient follow-up (GOTO)
Global Rapid Advanced Network Devoted to the Multi-messenger Addicts (GRANDMA)
Space-based multi-band astronomical Variable Objects Monitor (SVOM)
Research Team
Infrastructure
JUNO http://juno.ihep.cas.cn
CTA https://www.cta-observatory.org/
GOTO https://goto-observatory.org/
GRANDMA https://grandma.ijclab.in2p3.fr/
Svom https://www.svom.eu/en/the-svom-mission/
POLARBEAR https://cosmology.ucsd.edu/Polarbear
Collaborators
Kasetsart University, Thailand