Energy Reconstruction Methods in the IceCube Neutrino Telescope

Research output: Contribution to journal › Journal article › Research › peer-review

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Energy Reconstruction Methods in the IceCube Neutrino Telescope. / Aartsen, M.G.; Abbasi, R.; Ackermann, M.; Adams, J.; Aguilar, J.A.; Ahlers, M.; Altmann, D.; Arguelles, C.; Auffenberg, J.; Bai, X.; Baker, M.; Sarkar, Subir; Koskinen, David Jason.

In: Journal of Instrumentation, Vol. 9, P03009, 17.03.2014.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Aartsen, MG, Abbasi, R, Ackermann, M, Adams, J, Aguilar, JA, Ahlers, M, Altmann, D, Arguelles, C, Auffenberg, J, Bai, X, Baker, M, Sarkar, S & Koskinen, DJ 2014, 'Energy Reconstruction Methods in the IceCube Neutrino Telescope', Journal of Instrumentation, vol. 9, P03009. https://doi.org/10.1088/1748-0221/9/03/P03009

APA

Aartsen, M. G., Abbasi, R., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Altmann, D., Arguelles, C., Auffenberg, J., Bai, X., Baker, M., Sarkar, S., & Koskinen, D. J. (2014). Energy Reconstruction Methods in the IceCube Neutrino Telescope. Journal of Instrumentation, 9, [P03009]. https://doi.org/10.1088/1748-0221/9/03/P03009

Vancouver

Aartsen MG, Abbasi R, Ackermann M, Adams J, Aguilar JA, Ahlers M et al. Energy Reconstruction Methods in the IceCube Neutrino Telescope. Journal of Instrumentation. 2014 Mar 17;9. P03009. https://doi.org/10.1088/1748-0221/9/03/P03009

Author

Aartsen, M.G. ; Abbasi, R. ; Ackermann, M. ; Adams, J. ; Aguilar, J.A. ; Ahlers, M. ; Altmann, D. ; Arguelles, C. ; Auffenberg, J. ; Bai, X. ; Baker, M. ; Sarkar, Subir ; Koskinen, David Jason. / Energy Reconstruction Methods in the IceCube Neutrino Telescope. In: Journal of Instrumentation. 2014 ; Vol. 9.

Bibtex

@article{2088540c7b4a43de90b834efa5caebc5,
title = "Energy Reconstruction Methods in the IceCube Neutrino Telescope",
abstract = "Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov light produced by the transit through a medium of charged particles created in neutrino interactions. The amount of light emitted is proportional to the deposited energy, which is approximately equal to the neutrino energy for νe and νμ charged-current interactions and can be used to set a lower bound on neutrino energies and to measure neutrino spectra statistically in other channels. Here we describe methods and performance of reconstructing charged-particle energies and topologies from the observed Cherenkov light yield, including techniques to measure the energies of uncontained muon tracks, achieving average uncertainties in electromagnetic-equivalent deposited energy of ~15% above 10 TeV.",
author = "M.G. Aartsen and R. Abbasi and M. Ackermann and J. Adams and J.A. Aguilar and M. Ahlers and D. Altmann and C. Arguelles and J. Auffenberg and X. Bai and M. Baker and Subir Sarkar and Koskinen, {David Jason}",
year = "2014",
month = mar,
day = "17",
doi = "10.1088/1748-0221/9/03/P03009",
language = "English",
volume = "9",
journal = "Journal of Instrumentation",
issn = "1748-0221",
publisher = "Institute of Physics Publishing Ltd",

}

RIS

TY - JOUR

T1 - Energy Reconstruction Methods in the IceCube Neutrino Telescope

AU - Aartsen, M.G.

AU - Abbasi, R.

AU - Ackermann, M.

AU - Adams, J.

AU - Aguilar, J.A.

AU - Ahlers, M.

AU - Altmann, D.

AU - Arguelles, C.

AU - Auffenberg, J.

AU - Bai, X.

AU - Baker, M.

AU - Sarkar, Subir

AU - Koskinen, David Jason

PY - 2014/3/17

Y1 - 2014/3/17

N2 - Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov light produced by the transit through a medium of charged particles created in neutrino interactions. The amount of light emitted is proportional to the deposited energy, which is approximately equal to the neutrino energy for νe and νμ charged-current interactions and can be used to set a lower bound on neutrino energies and to measure neutrino spectra statistically in other channels. Here we describe methods and performance of reconstructing charged-particle energies and topologies from the observed Cherenkov light yield, including techniques to measure the energies of uncontained muon tracks, achieving average uncertainties in electromagnetic-equivalent deposited energy of ~15% above 10 TeV.

AB - Accurate measurement of neutrino energies is essential to many of the scientific goals of large-volume neutrino telescopes. The fundamental observable in such detectors is the Cherenkov light produced by the transit through a medium of charged particles created in neutrino interactions. The amount of light emitted is proportional to the deposited energy, which is approximately equal to the neutrino energy for νe and νμ charged-current interactions and can be used to set a lower bound on neutrino energies and to measure neutrino spectra statistically in other channels. Here we describe methods and performance of reconstructing charged-particle energies and topologies from the observed Cherenkov light yield, including techniques to measure the energies of uncontained muon tracks, achieving average uncertainties in electromagnetic-equivalent deposited energy of ~15% above 10 TeV.

U2 - 10.1088/1748-0221/9/03/P03009

DO - 10.1088/1748-0221/9/03/P03009

M3 - Journal article

VL - 9

JO - Journal of Instrumentation

JF - Journal of Instrumentation

SN - 1748-0221

M1 - P03009

ER -

ID: 129925517