All-sky Search for Time-integrated Neutrino Emission from Astrophysical Sources with 7 yr of IceCube Data

Collaboration
Sep 16, 2016
15 pages
Published in:
  • Astrophys.J. 835 (2017) 2, 151
  • Published: Jan 24, 2017
e-Print:
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Abstract: (IOP)
Since the recent detection of an astrophysical flux of high-energy neutrinos, the question of its origin has not yet fully been answered. Much of what is known about this flux comes from a small event sample of high neutrino purity, good energy resolution, but large angular uncertainties. In searches for point-like sources, on the other hand, the best performance is given by using large statistics and good angular reconstructions. Track-like muon events produced in neutrino interactions satisfy these requirements. We present here the results of searches for point-like sources with neutrinos using data acquired by the IceCube detector over 7 yr from 2008 to 2015. The discovery potential of the analysis in the northern sky is now significantly below Eν2dϕ/dEν{E}_{\nu }^{2}d\phi /{{dE}}_{\nu } = 10(−)(12) TeV cm(−)(2) s(−)(1), on average 38% lower than the sensitivity of the previously published analysis of 4 yr exposure. No significant clustering of neutrinos above background expectation was observed, and implications for prominent neutrino source candidates are discussed.
Note:
  • 19 pages, 17 figures, 3 tables; ; submitted to The Astrophysical Journal
  • astroparticle physics
  • galaxies: active
  • neutrinos
  • neutrino: interaction
  • neutrino: energy: high
  • IceCube
  • flux
  • energy resolution
  • sensitivity
  • performance