Abstract
- Received 8 November 2017
DOI:https://doi.org/10.1103/PhysRevLett.119.259902
© 2017 American Physical Society
Physics Subject Headings (PhySH)
Gravitation, Cosmology & Astrophysics
Erratum: Constraints on Ultrahigh-Energy Cosmic-Ray Sources from a Search for Neutrinos Above 10 PeV with IceCube [Phys. Rev. Lett. 117, 241101 (2016)]
M. G. Aartsen
Phys. Rev. Lett. 119, 259902 – Published 21 December 2017
Images
Figure 1
Model-dependent 90% confidence-level limits (solid lines) for cosmogenic and astrophysical neutrino predictions. The range of limits indicates the central 90% energy region. See the caption of the original Letter for full details.
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All-flavor-sum neutrino flux quasidifferential 90% C.L. upper limit on one energy decade flux windows (solid line). A model-dependent upper limit on an unbroken power-law flux from the current analysis () is also shown (dotted line). See the caption of the original Letter for full details.
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Constraints on the ultrahigh-energy cosmic-ray (UHECR) source evolution model and all flavor power-law flux model parameters. The colored areas represent parameter space excluded by the current analysis. (Top) Cosmogenic flux parameters and of UHECR-source cosmological evolution function of the form . (Bottom) Upper limits on power-law neutrino flux normalization and spectral cutoff energy . See the caption of the original Letter for full details.
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