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Chapter 3 Extra-galactic gamma-ray sources
Wang, Xiang-Yu1; Bi, Xiao-Jun2; Cao, Zhen2; Vallania, Piero3; Wu, Han-Rong2; Yan DH(闫大海)4; Yuan, Qiang5
发表期刊CHINESE PHYSICS C
2022-03
卷号46期号:3
DOI10.1088/1674-1137/ac3fa9
产权排序第4完成单位
收录类别SCI
关键词AGN Gamma-rays GRBs
摘要

Extra-galactic gamma-ray sources, such as gamma-ray bursts, active galactic nuclei, starburst galaxies, are interesting and important targets for LHAASO observations. In this chapter, the prospects of detecting these sources with LHAASO and their physical implications are studied. The upgrade plan for the Water Cherenkov Detector Array (WCDA), which aims to enhance the detectability of relatively lower energy photons, is also presented. In addition, a study on constraining the extragalactic background light with LHAASO observation of blazars is presented.

资助项目National Key R&D program of China[2018YFA0404203] ; National Natural Science Foundation Of China[12121003] ; National Natural Science Foundation Of China[11625312] ; China Manned Space Project[CMS-CSST-2021-B11]
项目资助者National Key R&D program of China[2018YFA0404203] ; National Natural Science Foundation Of China[12121003, 11625312] ; China Manned Space Project[CMS-CSST-2021-B11]
语种英语
学科领域天文学 ; 星系与宇宙学
文章类型Article
出版者IOP Publishing Ltd
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN1674-1137
URL查看原文
WOS记录号WOS:000819656800002
WOS研究方向Physics
WOS类目Physics, Nuclear ; Physics, Particles & Fields
关键词[WOS]EXTRAGALACTIC BACKGROUND LIGHT ; STAR-FORMING GALAXIES ; GEV EMISSION ; ARGO-YBJ ; FERMI OBSERVATIONS ; TEV EMISSION ; ENERGY ; SPECTRA ; CONSTRAINTS ; BLAZARS
引用统计
被引频次:4[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
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条目标识符http://ir.ynao.ac.cn/handle/114a53/24949
专题高能天体物理研究组
中国科学院天体结构与演化重点实验室
通讯作者Wang, Xiang-Yu
作者单位1.School of Astronomy and Space Sciences, Nanjing University, Nanjing 210093, China
2.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China
3.INAF - Osservatorio Astrofisico di Torino, Strada Osservatorio 20, 10025 Pino Torinese (TO), Italy and INFN Sezione di Torino, Via P. Giuria 1, 10125 Torino, Italy
4.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
5.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China
推荐引用方式
GB/T 7714
Wang, Xiang-Yu,Bi, Xiao-Jun,Cao, Zhen,et al. Chapter 3 Extra-galactic gamma-ray sources[J]. CHINESE PHYSICS C,2022,46(3).
APA Wang, Xiang-Yu.,Bi, Xiao-Jun.,Cao, Zhen.,Vallania, Piero.,Wu, Han-Rong.,...&Yuan, Qiang.(2022).Chapter 3 Extra-galactic gamma-ray sources.CHINESE PHYSICS C,46(3).
MLA Wang, Xiang-Yu,et al."Chapter 3 Extra-galactic gamma-ray sources".CHINESE PHYSICS C 46.3(2022).
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