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Search for very high energy gamma rays from possible ultra-high energy cosmic ray sources by the MAGIC Telescope

机译:从可能的超高能量中寻找非常高能量的伽马射线   maGIC望远镜的宇宙射线源

摘要

The origin of ultra-high energy (UHE) cosmic rays is still an open question.In the present work, we searched the possible UHE cosmic ray sources using theMAGIC telescope for the associated very high energy (VHE) gamma ray emission.Due to constrained propagation distance of such cosmic rays, we selected nearbygalaxies in vicinity of the direction of the AGASA triplet and a HiRes UHEcosmic ray event: NGC 3610 and NGC 3613 (quasar remnants); Arp 299 (a system ofcolliding galaxies). No significant excess in the VHE region was found foundfrom these objects or their surrounding region. At multi-100 GeV regime, theupper limits on fluxes were given against gamma ray sources in surroundingregion. The presented limits constrain the flux of a new hypothetical source inthe region, provided the cosmic rays are emitted from a single point-likeorigin.
机译:超高能(UHE)宇宙射线的起源仍然是一个悬而未决的问题。在目前的工作中,我们使用MAGIC望远镜搜索了可能的超高能(UHE)宇宙射线源,以寻找相关的超高能(VHE)伽玛射线发射。在此类宇宙射线的传播距离上,我们选择了在AGASA三重态和HiRes UHE宇宙射线事件附近的附近星系:NGC 3610和NGC 3613(类星体残余); Arp 299(一个碰撞星系系统)。从这些物体或其周围区域未发现VHE区域明显过剩。在多100 GeV体制下,通量的上限针对周围区域的伽马射线源。如果宇宙射线是从单个点状原点发出的,则提出的限制将限制该区域中新的假设源的通量。

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