All-sky Search for Time-integrated Neutrino Emission from Astrophysical Sources with 7 yr of IceCube Data
Collaboration
15 pages
Published in:
- Astrophys.J. 835 (2017) 2, 151
- Published: Jan 24, 2017
e-Print:
- 1609.04981 [astro-ph.HE]
Experiments:
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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 = 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
References(64)
Figures(17)