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dc.contributor.authorAartsen, M. G.
dc.contributor.authorBesson, David Zeke
dc.date.accessioned2020-06-18T21:17:20Z
dc.date.available2020-06-18T21:17:20Z
dc.date.issued2017-10-20
dc.identifier.citationAartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Al Samarai, I., Altmann, D., Andeen, K., Anderson, T., Ansseau, I., Anton, G., Archinger, M., Argüelles, C., Auffenberg, J., Axani, S., Bagherpour, H., Bai, X., Barwick, S. W., Baum, V., … Zoll, M. (2017). Measurement of the νμ energy spectrum with IceCube-79: IceCube Collaboration. The European physical journal. C, Particles and fields, 77(10), 692. https://doi.org/10.1140/epjc/s10052-017-5261-3en_US
dc.identifier.urihttp://hdl.handle.net/1808/30557
dc.descriptionThis work is licensed under a Creative Commons Attribution 4.0 International License.en_US
dc.description.abstractIceCube is a neutrino observatory deployed in the glacial ice at the geographic South Pole. The νμ energy unfolding described in this paper is based on data taken with IceCube in its 79-string configuration. A sample of muon neutrino charged-current interactions with a purity of 99.5% was selected by means of a multivariate classification process based on machine learning. The subsequent unfolding was performed using the software truee. The resulting spectrum covers an Eν-range of more than four orders of magnitude from 125 GeV to 3.2 PeV. Compared to the Honda atmospheric neutrino flux model, the energy spectrum shows an excess of more than 1.9σ in four adjacent bins for neutrino energies Eν≥177.8TeV. The obtained spectrum is fully compatible with previous measurements of the atmospheric neutrino flux and recent IceCube measurements of a flux of high-energy astrophysical neutrinos.en_US
dc.publisherSpringer Verlagen_US
dc.rights© The Author(s) 2017.en_US
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/en_US
dc.titleMeasurement of the νμ energy spectrum with IceCube-79en_US
dc.typeArticleen_US
kusw.kuauthorBesson, David Zeke
kusw.kudepartmentPhysics and Astronomyen_US
dc.identifier.doi10.1140/epjc/s10052-017-5261-3en_US
kusw.oaversionScholarly/refereed, publisher versionen_US
kusw.oapolicyThis item meets KU Open Access policy criteria.en_US
dc.identifier.pmidPMC6956919en_US
dc.rights.accessrightsopenAccessen_US


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© The Author(s) 2017.
Except where otherwise noted, this item's license is described as: © The Author(s) 2017.