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.
Universe evolution [Credit: NASA/WMAP]
Image of black hole [Credit: EHT]
Active Galactic Nuclei (AGN) [Credit: NASA/JPL]
Cosmic Microwave Background (CMB)
[Credit: MIT]
Research team
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1) Dr. Apimook Watcharangkool |
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(Coordinator) |
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2) Dr. Utane Sawangwit |
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3) Dr. Siraprapa Sanpa-arsa |
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4) Dr. Anirut Phriksee |
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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.
- University of Portsmouth, U.K.
- University of Manchester, U.K.
- Guangzhou University, China
- National Astronomical Observatory of China
- Institute of High Energy Physics, China