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@ARTICLE{Collaboration:398611,
      author       = {Aartsen, M. G. and Ackermann, M. and Adams, J. and Aguilar,
                      J. A. and Ahlers, M. and Ahrens, M. and Samarai, I. Al and
                      Altmann, D. and Andeen, K. and Anderson, T. and Ansseau, I.
                      and Anton, G. and Argüelles, C. and Auffenberg, J. and
                      Axani, S. and Bagherpour, H. and Bai, X. and Barron, J. P.
                      and Barwick, S. W. and Baum, V. and Bay, R. and Beatty, J.
                      J. and Tjus, J. Becker and Becker, K. -H. and BenZvi, S. and
                      Berley, D. and Bernardini, E. and Besson, D. Z. and Binder,
                      G. and Bindig, D. and Blaufuss, E. and Blot, S. and Bohm, C.
                      and Börner, M. and Bos, F. and Bose, D. and Böser, S. and
                      Botner, O. and Bourbeau, J. and Bradascio, F. and Braun, J.
                      and Brayeur, L. and Brenzke, M. and Bretz, Hans-Peter and
                      Bron, S. and Brostean-Kaiser, J. and Burgman, A. and Carver,
                      T. and Casey, J. and Casier, M. and Cheung, E. and Chirkin,
                      D. and Christov, A. and Clark, K. and Classen, L. and
                      Coenders, S. and Collin, G. H. and Conrad, J. M. and Cowen,
                      D. F. and Cross, R. and Day, M. and de André, J. P. A. M.
                      and De Clercq, C. and DeLaunay, J. J. and Dembinski, H. and
                      De Ridder, S. and Desiati, P. and de Vries, K. D. and de
                      Wasseige, G. and de With, M. and DeYoung, T. and
                      Díaz-Vélez, J. C. and di Lorenzo, V. and Dujmovic, H. and
                      Dumm, J. P. and Dunkman, M. and Eberhardt, B. and Ehrhardt,
                      T. and Eichmann, B. and Eller, P. and Evenson, P. A. and
                      Fahey, S. and Fazely, A. R. and Felde, J. and Filimonov, K.
                      and Finley, C. and Flis, S. and Franckowiak, A. and
                      Friedman, E. and Fuchs, T. and Gaisser, T. K. and Gallagher,
                      J. and Gerhardt, L. and Ghorbani, K. and Giang, W. and
                      Glauch, T. and Glüsenkamp, T. and Goldschmidt, A. and
                      Gonzalez, J. G. and Grant, D. and Griffith, Z. and Haack, C.
                      and Hallgren, A. and Halzen, F. and Hanson, K. and Hebecker,
                      D. and Heereman, D. and Helbing, K. and Hellauer, R. and
                      Hickford, S. and Hignight, J. and Hill, G. C. and Hoffman,
                      K. D. and Hoffmann, R. and Hokanson-Fasig, B. and Hoshina,
                      K. and Huang, F. and Huber, M. and Hultqvist, K. and
                      Hünnefeld, M. and In, S. and Ishihara, A. and Jacobi, E.
                      and Japaridze, G. S. and Jeong, M. and Jero, K. and Jones,
                      B. J. P. and Kalaczynski, P. and Kang, W. and Kappes, A. and
                      Karg, T. and Karle, A. and Katz, U. and Kauer, M. and
                      Keivani, A. and Kelley, J. L. and Kheirandish, A. and Kim,
                      J. and Kim, M. and Kintscher, T. and Kiryluk, J. and
                      Kittler, T. and Klein, S. R. and Kohnen, G. and Koirala, R.
                      and Kolanoski, H. and Köpke, L. and Kopper, C. and Kopper,
                      S. and Koschinsky, J. P. and Koskinen, D. J. and Kowalski,
                      M. and Krings, K. and Kroll, M. and Krückl, G. and Kunnen,
                      J. and Kunwar, S. and Kurahashi, N. and Kuwabara, T. and
                      Kyriacou, A. and Labare, M. and Lanfranchi, J. L. and
                      Larson, M. J. and Lauber, F. and Lennarz, D. and
                      Lesiak-Bzdak, M. and Leuermann, M. and Liu, Q. R. and Lu, L.
                      and Lünemann, J. and Luszczak, W. and Madsen, J. and Maggi,
                      G. and Mahn, K. B. M. and Mancina, S. and Maruyama, R. and
                      Mase, K. and Maunu, R. and McNally, F. and Meagher, K. and
                      Medici, M. and Meier, M. and Menne, T. and Merino, G. and
                      Meures, T. and Miarecki, S. and Micallef, J. and Momenté,
                      G. and Montaruli, T. and Moore, R. W. and Moulai, M. and
                      Nahnhauer, R. and Nakarmi, P. and Naumann, U. and Neer, G.
                      and Niederhausen, H. and Nowicki, S. C. and Nygren, D. R.
                      and Pollmann, A. Obertacke and Olivas, A. and O'Murchadha,
                      A. and Palczewski, T. and Pandya, H. and Pankova, D. V. and
                      Peiffer, P. and Pepper, J. A. and Heros, C. Pérez de los
                      and Pieloth, D. and Pinat, E. and Plum, M. and Price, P. B.
                      and Przybylski, G. T. and Raab, C. and Rädel, L. and
                      Rameez, M. and Rawlins, K. and Rea, I. C. and Reimann, R.
                      and Relethford, B. and Relich, M. and Resconi, E. and Rhode,
                      W. and Richman, M. and Robertson, S. and Rongen, M. and
                      Rott, C. and Ruhe, T. and Ryckbosch, D. and Rysewyk, D. and
                      Sälzer, T. and Herrera, S. E. Sanchez and Sandrock, A. and
                      Sandroos, J. and Sarkar, S. and Sarkar, S. and Satalecka, K.
                      and Schlunder, P. and Schmidt, T. and Schneider, A. and
                      Schoenen, S. and Schöneberg, S. and Schumacher, L. and
                      Seckel, D. and Seunarine, S. and Soedingrekso, J. and
                      Soldin, D. and Song, M. and Spiczak, G. M. and Spiering, C.
                      and Stachurska, J. and Stamatikos, M. and Stanev, T. and
                      Stasik, A. and Stettner, J. and Steuer, A. and Stezelberger,
                      T. and Stokstad, R. G. and Stößl, A. and Strotjohann, N.
                      L. and Sullivan, G. W. and Sutherland, M. and Taboada, I.
                      and Tatar, J. and Tenholt, F. and Ter-Antonyan, S. and
                      Terliuk, A. and Tešić, G. and Tilav, S. and Toale, P. A.
                      and Tobin, M. N. and Toscano, S. and Tosi, D. and
                      Tselengidou, M. and Tung, C. F. and Turcati, A. and Turley,
                      C. F. and Ty, B. and Unger, E. and Usner, M. and
                      Vandenbroucke, J. and Van Driessche, W. and van Eijndhoven,
                      N. and Vanheule, S. and van Santen, J. and Vehring, M. and
                      Vogel, E. and Vraeghe, M. and Walck, C. and Wallace, A. and
                      Wallraff, M. and Wandler, F. D. and Wandkowsky, N. and Waza,
                      A. and Weaver, C. and Weiss, M. J. and Wendt, C. and
                      Werthebach, J. and Westerhoff, S. and Whelan, B. J. and
                      Wiebe, K. and Wiebusch, C. H. and Wille, L. and Williams, D.
                      R. and Wills, L. and Wolf, M. and Wood, J. and Wood, T. R.
                      and Woolsey, E. and Woschnagg, K. and Xu, D. L. and Xu, X.
                      W. and Xu, Y. and Yanez, J. P. and Yodh, G. and Yoshida, S.
                      and Yuan, T. and Zoll, M.},
      collaboration = {{IceCube Collaboration}},
      title        = {{M}easurement of {A}tmospheric {N}eutrino {O}scillations at
                      6-56 {G}e{V} with {I}ce{C}ube {D}eep{C}ore},
      reportid     = {PUBDB-2018-00002, arXiv:1707.07081},
      year         = {2017},
      note         = {8 pages, 3 figures},
      abstract     = {We present a measurement of the atmospheric neutrino
                      oscillation parameters using three years of data from the
                      IceCube Neutrino Observatory. The DeepCore infill array in
                      the center of IceCube enables detection and reconstruction
                      of neutrinos produced by the interaction of cosmic rays in
                      the Earth's atmosphere at energies as low as $\sim5$ GeV.
                      That energy threshold permits measurements of muon neutrino
                      disappearance, over a range of baselines up to the diameter
                      of the Earth, probing the same range of $L/E_\nu$ as
                      long-baseline experiments but with substantially higher
                      energy neutrinos. This analysis uses neutrinos from the full
                      sky with reconstructed energies from $5.6$ - $56$ GeV. We
                      measure $\Delta m^2_{32}=2.31^{+0.11}_{-0.13} \times
                      10^{-3}$ eV$^2$ and $\sin^2
                      \theta_{23}=0.51^{+0.07}_{-0.09}$, assuming normal neutrino
                      mass ordering. These results are consistent with, and of
                      similar precision to, those from accelerator and
                      reactor-based experiments.},
      cin          = {ZEU-ICE},
      cid          = {I:(DE-H253)ZEU-ICE-20160806},
      pnm          = {613 - Matter and Radiation from the Universe (POF3-613)},
      pid          = {G:(DE-HGF)POF3-613},
      experiment   = {EXP:(DE-H253)IceCube-20150101},
      typ          = {PUB:(DE-HGF)25 / PUB:(DE-HGF)29},
      eprint       = {1707.07081},
      howpublished = {arXiv:1707.07081},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1707.07081;\%\%$},
      doi          = {10.3204/PUBDB-2018-00002},
      url          = {https://bib-pubdb1.desy.de/record/398611},
}