Search for TeV gamma rays emission from the shell-like SNR G40.5-0.5 using the Yangbajing extensive air shower array

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	Search for TeV gamma rays emission from the shell-like SNR G40.5-0.5 using the Yangbajing extensive air shower array
	Asy 合作组
刊名	HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION
	2006
卷号	30 期号:1 页码:#REF!
关键词	extensive air shower gamma rays shell-like supernova remnants EGRET unidentified source
通讯作者	Zhang, JL (reprint author), CAS, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China.
英文摘要	Using observation data of the Yangbajing extensive air shower array from October 2000 to September 2001, the TeV gamma rays from the shell-like SNR G40.5-0.5 direction were detected. A region with the highest excess of 4.4 sigma was found using two dimensional analysis method. The position of EGRET unidentified source GeV J1907+0557 is near the centrer of the region.
学科主题	Physics
类目[WOS]	Physics, Nuclear ; Physics, Particles & Fields
收录类别	SCI
WOS记录号	WOS:000234460500002
公开日期	2016-05-03
内容类型	期刊论文
源URL	[http://ir.ihep.ac.cn/handle/311005/225495]
专题	高能物理研究所_粒子天体物理中心
推荐引用方式 GB/T 7714	Asy 合作组. Search for TeV gamma rays emission from the shell-like SNR G40.5-0.5 using the Yangbajing extensive air shower array[J]. HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,2006,30(1):#REF!.
APA	Asy 合作组.(2006).Search for TeV gamma rays emission from the shell-like SNR G40.5-0.5 using the Yangbajing extensive air shower array.HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION,30(1),#REF!.
MLA	Asy 合作组."Search for TeV gamma rays emission from the shell-like SNR G40.5-0.5 using the Yangbajing extensive air shower array".HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS-CHINESE EDITION 30.1(2006):#REF!.