Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

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Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data. / Aartsen, M.G.; Ackermann, M.; Adams, J.; Aguilar, J.A.; Ahlers, M.; Ahrens, M.; Altmann, D.; Anderson, T.; Arguelles, C.; Arlen, T.C.; Auffenberg, J.; Koskinen, David Jason; Larson, Michael James; Sarkar, Subir.

In: Physical Review Letters, Vol. 113, No. 10, 101101, 02.09.2014.

Research output: Contribution to journalJournal articleResearchpeer-review

Harvard

Aartsen, MG, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Ahrens, M, Altmann, D, Anderson, T, Arguelles, C, Arlen, TC, Auffenberg, J, Koskinen, DJ, Larson, MJ & Sarkar, S 2014, 'Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data', Physical Review Letters, vol. 113, no. 10, 101101. https://doi.org/10.1103/PhysRevLett.113.101101

APA

Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., Anderson, T., Arguelles, C., Arlen, T. C., Auffenberg, J., Koskinen, D. J., Larson, M. J., & Sarkar, S. (2014). Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data. Physical Review Letters, 113(10), [101101]. https://doi.org/10.1103/PhysRevLett.113.101101

Vancouver

Aartsen MG, Ackermann M, Adams J, Aguilar JA, Ahlers M, Ahrens M et al. Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data. Physical Review Letters. 2014 Sep 2;113(10). 101101. https://doi.org/10.1103/PhysRevLett.113.101101

Author

Aartsen, M.G. ; Ackermann, M. ; Adams, J. ; Aguilar, J.A. ; Ahlers, M. ; Ahrens, M. ; Altmann, D. ; Anderson, T. ; Arguelles, C. ; Arlen, T.C. ; Auffenberg, J. ; Koskinen, David Jason ; Larson, Michael James ; Sarkar, Subir. / Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data. In: Physical Review Letters. 2014 ; Vol. 113, No. 10.

Bibtex

@article{909abc9f31a14985b6a005d0882219ab,
title = "Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data",
abstract = "A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012–2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV–PeV range at the level of 10^-8  GeV cm^-2 s^-1 sr^-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotropic arrival directions, suggesting either numerous or spatially extended sources. The three-year data set, with a live time of 988 days, contains a total of 37 neutrino candidate events with deposited energies ranging from 30 to 2000 TeV. The 2000-TeV event is the highest-energy neutrino interaction ever observed.",
author = "M.G. Aartsen and M. Ackermann and J. Adams and J.A. Aguilar and M. Ahlers and M. Ahrens and D. Altmann and T. Anderson and C. Arguelles and T.C. Arlen and J. Auffenberg and Koskinen, {David Jason} and Larson, {Michael James} and Subir Sarkar",
year = "2014",
month = sep,
day = "2",
doi = "10.1103/PhysRevLett.113.101101",
language = "English",
volume = "113",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "10",

}

RIS

TY - JOUR

T1 - Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

AU - Aartsen, M.G.

AU - Ackermann, M.

AU - Adams, J.

AU - Aguilar, J.A.

AU - Ahlers, M.

AU - Ahrens, M.

AU - Altmann, D.

AU - Anderson, T.

AU - Arguelles, C.

AU - Arlen, T.C.

AU - Auffenberg, J.

AU - Koskinen, David Jason

AU - Larson, Michael James

AU - Sarkar, Subir

PY - 2014/9/2

Y1 - 2014/9/2

N2 - A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012–2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV–PeV range at the level of 10^-8  GeV cm^-2 s^-1 sr^-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotropic arrival directions, suggesting either numerous or spatially extended sources. The three-year data set, with a live time of 988 days, contains a total of 37 neutrino candidate events with deposited energies ranging from 30 to 2000 TeV. The 2000-TeV event is the highest-energy neutrino interaction ever observed.

AB - A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012–2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV–PeV range at the level of 10^-8  GeV cm^-2 s^-1 sr^-1 per flavor and reject a purely atmospheric explanation for the combined three-year data at 5.7σ. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotropic arrival directions, suggesting either numerous or spatially extended sources. The three-year data set, with a live time of 988 days, contains a total of 37 neutrino candidate events with deposited energies ranging from 30 to 2000 TeV. The 2000-TeV event is the highest-energy neutrino interaction ever observed.

U2 - 10.1103/PhysRevLett.113.101101

DO - 10.1103/PhysRevLett.113.101101

M3 - Journal article

C2 - 25238345

VL - 113

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 10

M1 - 101101

ER -

ID: 124373802