A New Method for Finding Point Sources in High-energy Neutrino Data

Abstract

The IceCube collaboration has reported the first detection of high-energy astrophysical neutrinos including $\sim 50$ high-energy starting events, but no individual sources have been identified. It is therefore important to develop the most sensitive and efficient possible algorithms to identify point sources of these neutrinos. The most popular current method works by exploring a dense grid of possible directions to individual sources, and identifying the single direction with the maximum probability of having produced multiple detected neutrinos. This method has numerous strengths, but it is computationally intensive and, because it focuses on the single best location for a point source, additional point sources are not included in the evidence. We propose a new maximum likelihood method that uses the angular separations between all pairs of neutrinos in the data. Unlike existing autocorrelation methods for this type of analysis, which also use angular separations between neutrino pairs, our method incorporates information about the point spread function and can identify individual point sources. We find that if the angular resolution is a few degrees or better, then this approach reduces both false positive and false negative errors compared to the current method, and is also more computationally efficient up to, potentially, hundreds of thousands of detected neutrinos.

6 pages, 3 figures, published in the Astrophysical Journal

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• High-energy neutrinos from sources in clusters of galaxies
• Identifying Ultrahigh-Energy Cosmic-Ray Accelerators with Future Ultrahigh-Energy Neutrino Detectors
• IC at IC: IceCube can constrain the intrinsic charm of the proton
• Detection prospects for high energy neutrino sources from the anisotropic matter distribution in the local universe
• Near-future discovery of point sources of ultra-high-energy neutrinos
• Observational strategies for ultrahigh-energy neutrinos: the importance of deep sensitivity for detection and astronomy