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
{"title":"New generation Cherenkov telescope array: HADAR and its performance introduction","authors":"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":"10.1016/j.nuclphysb.2025.116935","DOIUrl":null,"url":null,"abstract":"<div><div>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.</div></div>","PeriodicalId":54712,"journal":{"name":"Nuclear Physics B","volume":"1017 ","pages":"Article 116935"},"PeriodicalIF":2.5000,"publicationDate":"2025-04-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Nuclear Physics B","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0550321325001440","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"PHYSICS, PARTICLES & FIELDS","Score":null,"Total":0}
引用次数: 0
Abstract
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.
期刊介绍:
Nuclear Physics B focuses on the domain of high energy physics, quantum field theory, statistical systems, and mathematical physics, and includes four main sections: high energy physics - phenomenology, high energy physics - theory, high energy physics - experiment, and quantum field theory, statistical systems, and mathematical physics. The emphasis is on original research papers (Frontiers Articles or Full Length Articles), but Review Articles are also welcome.