Nuclear Physics B (Aug 2025)

New generation Cherenkov telescope array: HADAR and its performance introduction

  • Qingyuan Hou,
  • Qingqian Zhou,
  • Tianlu Chen,
  • Youliang Feng,
  • Hengjiao Liu,
  • Yiqing Guo,
  • Cheng Liu,
  • Zihao Zhang,
  • Xinlong Li,
  • Qi Gao,
  • Maoyuan Liu,
  • Xiangli Qian,
  • Yuanqi Liu,
  • Jiadan Xie,
  • Shanjie Shu,
  • Weiqi Han,
  • Qijiao Fang,
  • Yanan Wang,
  • Shaohua Zhang

DOI
https://doi.org/10.1016/j.nuclphysb.2025.116935
Journal volume & issue
Vol. 1017
p. 116935

Abstract

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Astrophysical very high energy (VHE) gamma-rays are believed to result almost exclusively from the interactions of populations of highly relativistic particles with ambient matter or photon fields. The study of these VHE photons therefore allows us to examine the processes of particle acceleration in the Universe, and the extreme environments in which they occur.To explore the origins and properties of gamma-rays, the High Altitude Detection of Astronomical Radiation (HADAR) experiment has been proposed to study these events. The refractive atmospheric Cherenkov telescope, a key component of HADAR, features a wide field of view (FOV) and exceptional sensitivity. It is designed to indirectly detect gamma-rays by capturing Cherenkov radiation produced by extensive air showers initiated by primary gamma-rays. This study concentrates on the design and performance parameters of the refractive atmospheric Cherenkov telescope array.

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