文摘HADAR(High Altitude Detection of Astronomical Radiation)是一个基于大气切伦科夫成像技术的地面望远镜阵列,其采用大口径折射式水透镜系统来收集大气切伦科夫光,以实现对10 GeV—10 TeV能量段的伽马射线和宇宙线的探测.HADAR具有低阈能和大视场的优势,因此可以对天区进行连续扫描和观测,在观测活动星系核(Active Galactic Nuclei,AGN)等银河系外伽马射线源方面具有明显优势.本文研究了HADAR实验对AGN的探测能力.基于费米望远镜(Fermi Large Area Telescope,Fermi-LAT)的AGN源能谱信息,将观测能量外推至甚高能能段,同时加入河外背景光的吸收效应,以计算HADAR对AGN源观测的统计显著性.研究结果显示,HADAR运行一年时间,预计将有31个Fermi-LAT AGN源以高于5倍显著性被观测到,其中大部分为蝎虎状天体类型.
基金supported by Shanghai Jiao Tong University 2030 Initiative,Science and Technology Commission of Shanghai Municipality project (No.23JC1410200)Zhangjiang National Innovation Demonstration Zone project (No.ZJ2023-ZD-003)+7 种基金supported by the China-Chile Joint Research Fund under project CCJRF 2205, by FONDECYT grant 1201371the ANID BASAL project FB210003.YZC is supported by the National Natural Science Foundation of China (NSFC, Grant No.12303054)the Yunnan Fundamental Research Projects (Grant No.202401AU070063)the International Centre of Supernovae,Yunnan Key Laboratory (No.202302AN360001)supported by the NSFC (Grant No.12150009)supported by the NSFC through grants 12173029 and 12233013supported by the NSFC (Grant No.12120101003 and 12233008)supported by the NSFC (Grant No.12233003)