首页> 外文会议>Proceedings of the 32nd International Cosmic Ray Conference >Neutrino triggered high-energy gamma-ray follow-up with IceCube
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Neutrino triggered high-energy gamma-ray follow-up with IceCube

机译:中微子通过IceCube触发了高能伽马射线跟踪

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We present the status of a program for the generation of online alerts issued by IceCube for gamma-rayfollow-up observations by Air Shower Cherenkov telescopes (e.g. MAGIC). To overcome the low probability ofsimultaneous observations of flares of objects with gamma-ray and neutrino telescopes a neutrino triggered follow-upscheme is developed. This mode of operation aims at increasing the availability of simultaneous multi-messenger datawhich can increase the discovery potential and constrain the phenomenological interpretation of the high energy emissionof selected source classes (e.g. blazars). This requires a fast and stable online analysis of potential neutrino signals. Wepresent the work on a significance based alert scheme for a list of phenomenologically selected sources. To monitor thedetector and the alert system reliability, monitoring systems have been implemented on different levels. We show datafrom the first weeks of running this system.
机译:我们介绍了IceCube发出的在线警报生成程序的状态,该警报用于通过Air Shower Cherenkov望远镜(例如MAGIC)进行的伽马射线跟踪观测。为了克服用伽马射线和中微子望远镜同时观测目标耀斑的低概率,开发了一种中微子触发的跟踪方案。这种操作模式旨在提高同时使用的多信使数据的可用性,这可以增加发现潜力,并限制对选定源类别(例如blazars)的高能量排放的现象学解释。这需要对潜在的中微子信号进行快速,稳定的在线分析。我们介绍了基于显着性的警报方案的工作,这些警报方案用于从现象学中选择的来源列表。为了监视检测器和警报系统的可靠性,已在不同级别上实施了监视系统。我们显示了运行该系统的前几周的数据。

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