Ten years of All-sky Neutrino Point-SourceSearches

T. Carver
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引用次数: 4

Abstract

These proceedings present the results of point-like neutrino source searches using ~10 yrs of IceCube data from Apr.~6, 2008 to Jul.~10, 2018. We evaluate the significance of an astrophysical signal from a point-like source looking for an excess of clustered neutrino events with energies above ~1 TeV among the background of atmospheric muons and neutrinos. We perform a full sky scan, a search based on a selected source catalog, and a catalog population study. The most significant location in the Northern hemisphere from the full-sky scan is compatible with the Seyfert galaxy NGC 1068. This object had also been identified in the source catalog search which finds a 2.9 $\sigma$ excess after accounting for statistical trials. The combination of this result along with excesses observed at the coordinates of three other sources, including TXS 0506+056, suggests that collectively correlations with sources in the Northern catalog are inconsistent with background at the level of 3.3 $\sigma$. These results motivate further interest in such point-like sources which should become observable or ruled out after accumulation of more data or with future detectors.
10年的全天中微子点源研究
这些论文展示了利用冰立方从2008年4月6日到2018年7月10日的10年数据进行的点状中微子源搜索的结果。我们评估了在大气介子和中微子背景中寻找能量高于~1 TeV的过量聚集中微子事件的天体物理信号的意义。我们执行一个完整的天空扫描,一个搜索基于一个选定的源目录,和一个目录人口研究。在北半球的全天扫描中,最重要的位置与塞弗特星系ngc1068兼容。这个天体也在源目录搜索中被发现,在统计试验后发现2.9 $\sigma$超额。结合这一结果以及在其他三个源(包括TXS 0506+056)坐标上观察到的过量,表明与北方星表源的总体相关性与背景在3.3 $\sigma$水平上不一致。这些结果激发了人们对这种点状源的进一步兴趣,这种点状源应该在积累更多数据或使用未来的探测器之后才能被观察到或排除。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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