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.

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

Facilities

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

Suranaree University of Technology, Thailand

Chulalongkorn University, Thailand

Srinakharinwirot University, Thailand

Chiangmai University, Thailand

Khon Kaen University, Thailand

Mae Fah Luang University, Thailand

University of Durham, U.K.

มหาวิทยาลัยแห่ง Sheffield (สหราชอาณาจักร)

UKATC (สหราชอาณาจักร)