Speaker
Prof.
Huang Jing huangjing
(Institute of High Energy Physics, CAS)
Description
We have built a prototype of stereoscopic water Cherenkov detector array (SWCDA) inside the Tibet ASgamma air-shower array (Tibet-III array) by the end of 2024. The SWCDA project is the next generation of innovative ground-based stereoscopic water Cherenkov detection array, its main scientific goal is to observe 100GeV-10TeV high-energy gamma-ray astronomy, such as observation of blazars, active galactic nuclei (AGN/ AGN flare) and gamma-ray bursts (GRBs). This report will describe the observation results of prototype experiments of stereoscopic water Cherenkov detection array in detail.
Author
Prof.
Huang Jing huangjing
(Institute of High Energy Physics, CAS)
Co-authors
Prof.
Ding Chen
Dr
K.Y. Hu
Dr
L.M. Zhai
Dr
S.Y. Huang
Dr
Xu Chen
Dr
Y. Meng
Dr
Y.H. Zou
(Institute of High Energy Physics, CAS)
Y.L. Yu
(Institute of High Energy Physics, CAS)
Dr
Y.Y. Li
(Institute of High Energy Physics, CAS)
Dr
Ying Zhang
(Institute of High Energy Physics, CAS)
