% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@ARTICLE{Aartsen:316908,
      author       = {Aartsen, M. G. and Abraham, K. and Ackermann, Markus and
                      Adams, J. and Aguilar, J. A. and Ahlers, M. and Ahrens, M.
                      and Altmann, D. and Anderson, T. and Ansseau, I. and
                      Archinger, M. and Arguelles, C. and T. C. Arlen, T. C. and
                      Auffenberg, J. and Bai, X. and Barwick, S. W. and Baum, V.
                      and Bay, R. and Beatty, J. J. and Becker Tjus, J. and
                      Becker, K. H. and Beiser, E. and Berghaus, P. and Berley, D.
                      and Bernardini, E. and Bernhard, A. and Besson, D. Z. and
                      Binder, G. and Bindig, D. and Bissok, M. and Blaufuss, E.
                      and Blumenthal, J. and Boersma, D. J. and Bohm, C. and
                      Börner, M. and Bos, F. and Bose, D. and Böser, S. and
                      Botner, O. and Braun, J. and Brayeur, L. and Bretz, H. P.
                      and Buzinsky, N. 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 Cruz Silva, A. H. and Daughhetee, J. and
                      Davis, J. C. and Day, M. and de André, J. P. A. M. and De
                      Clercq, C. and del Pino Rosendo, E. 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 Dumman, J. P. and
                      Dunkman, M. and Eberhardt, B. and Ehrhardt, T. and Eichmann,
                      B. and Euler, S. and Evenson, P. A. and Fahey, S. and
                      Fazely, A. R. and Feintzeig, J. and Felde, J. and Filimonov,
                      K. and Finley, C. and Flis, S. and Fösig, C. C. and Fuchs,
                      T. and Gaisser, T. K. and Gaior, R. and Gallagher, J. and
                      Gerhardt, L. and Ghorbani, K. and Gier, D. and Gladstone, L.
                      and Glagla, M. and Glüsenkamp, T. and Goldschmidt, A. and
                      Golup, G. and Gonzalez, J. G. and Góra, D. and Grant, D.
                      and Griffith, Z. and Groß, A. and Ha, C. and Haack, C. and
                      Haj Ismail, A. and Hallgren, A. and Halzen, F. and Hansen,
                      E. and Hansmann, B. 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 Holzapfel, K. and Homeier, A. and Hoshina,
                      K. and Huang, F. and Huber, M. and Huelsnitz, W. and Hulth,
                      P. O. and Hultqvist, K. 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 Jurkovic, M. and Kappes, A. and
                      Karg, T. and Karle, A. and Kauer, M. and Keivani, A. and
                      Kelley, J. L. and Kemp, j. and Kheirandish, A. and Kiryluk,
                      J. and Klein, S. R. and Kohnen, G. and Koirala, R. and
                      Kolanoski, H. and Konietz, R. and Köpke, L. and Kopper, C.
                      and Kopper, S. and Koskinen, D. J. and Kowalski, Marek and
                      Krings, K. and Kroll, G. and Kroll, M. and Krückl, G. and
                      Kunnen, J. and Kurahashi, N. and Kuwabara, T. and Labare, M.
                      and Lanfranchi, J. L. and Larson, M. J. and Lesiak-Bzdak, M.
                      and Leuermann, M. and Leuner, J. and Lu, L. and Lünemann,
                      J. and Madsen, J. and Maggi, G. and Mahn, K. B. M. and
                      Mandelartz, M. and Maruyama, R. and Mase, K. and Matis, H.
                      S. and Maunu, R. and McNally, F. and Meagher, K. and Medici,
                      M. and Meli, A. and Menne, T. and Merino, G. and Meures, T.
                      and Miarecki, S. and Middell, E. and Mohrmann, L. and
                      Montaruli, T. and Morse, R. and Nahnhauer, R. and Naumann,
                      U. and Neer, G. and Niederhausen, H. and Nowicki, S. C. and
                      Nygren, D. R. and Obertacke Pollmann, A. and Olivas, A. and
                      Omairat, A. and O'Murchadha, A. and Palczewski, T. and
                      Pandya, H. and Pankova, D. V. and Paul, L. and Pepper, J. A.
                      and Pérez de los Heros, C. and Pfendner, C. and Pieloth, D.
                      and Pinat, E. and Posselt, J. and Price, P. B. and
                      Przybylski, G. T. and Quinnan, M. and Raab, C. and Rädel,
                      L. and Rameez, M. and Rawlins, K. and Reimann, R. and
                      Relich, M. and Resconi, E. and Rhode, W. and Richman, M. and
                      Richter, S. and Riedel, B. and Robertson, S. and Rongen, M.
                      and Rott, C. and Ruhe, T. and Ryckbosch, D. and Sabbatini,
                      L. and Sander, H. G. and Sandrock, A. and Sandroos, J. and
                      Sarkar, S. and Schatto, K. and Schimp, M. and Schmidt, T.
                      and Schoenen, S. and Schöneberg, S. and Schönwald, A. and
                      Schulte, L. and Schumacher, L. and Seckel, D. and Seunarine,
                      S. and Soldin, D. and Song, M. and Spiczak, G. M. and
                      Spiering, C. and Stahlberg, M. and Stamatikos, M. and
                      Stanev, T. and Stasik, A. and Steuer, A. and Stezelberger,
                      T. and Stokstad, R. G. and Stößl, A. and Ström, R. and
                      Strotjohann, N. L. and Sullivan, G. W. and Sutherland, M.
                      and Taavola, H. and Taboada, I. and Tatar, J. and
                      Ter-Antonyan, S. and Terliuk, A. and Tesic, G. and Tilav, S.
                      and Toale, P. A. and Tobin, M. N. and Toscano, S. and Tosi,
                      D. and Tselengidou, M. and Turcati, A. and Unger, E. and
                      Usner, M. and Vallecorsa, S. and Vandenbroucke, J. and van
                      Eijndhoven, N. and Vanheule, S. and van Santen, J. and
                      Veenkamp, J. and Vehring, M. and Voge, M. and Vraeghe, M.
                      and Walck, C. and Wallace, A. and Wallraff, M. and
                      Wandkowsky, N. and Weaver, Ch. and Wendt, C. 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 Wissing, H.
                      and Wolf, M. and Wood, T. R. 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 Zoll, M.},
      title        = {{N}eutrino oscillation studies with
                      {I}ce{C}ube-{D}eep{C}ore},
      journal      = {Nuclear physics / B},
      volume       = {908},
      issn         = {0550-3213},
      address      = {Amsterdam},
      publisher    = {North-Holland Publ. Co.},
      reportid     = {PUBDB-2017-00278},
      pages        = {161 - 177},
      year         = {2016},
      abstract     = {IceCube, a gigaton-scale neutrino detector located at the
                      South Pole, was primarily designed to search for
                      astrophysical neutrinos with energies of PeV and higher.
                      This goal has been achieved with the detection of the
                      highest energy neutrinos to date. At the other end of the
                      energy spectrum, the DeepCore extension lowers the energy
                      threshold of the detector to approximately 10 GeV and opens
                      the door for oscillation studies using atmospheric
                      neutrinos. An analysis of the disappearance of these
                      neutrinos has been completed, with the results produced
                      being complementary with dedicated oscillation experiments.
                      Following a review of the detector principle and
                      performance, the method used to make these calculations, as
                      well as the results, is detailed. Finally, the future
                      prospects of IceCube-DeepCore and the next generation of
                      neutrino experiments at the South Pole (IceCube-Gen2,
                      specifically the PINGU sub-detector) are briefly discussed.},
      keywords     = {neutrino nucleon: interaction (INSPIRE) / neutrino:
                      oscillation (INSPIRE) / neutrino: mixing angle (INSPIRE) /
                      neutrino: mass difference (INSPIRE) / neutrino: detector
                      (INSPIRE) / neutrino: energy (INSPIRE) / neutrino:
                      atmosphere (INSPIRE) / energy: threshold (INSPIRE) / pole
                      (INSPIRE) / neutrino: energy spectrum (INSPIRE) /
                      performance (INSPIRE) / IceCube (INSPIRE) / PINGU (INSPIRE)
                      / experimental results (INSPIRE)},
      cin          = {ZEU-ICE},
      ddc          = {530},
      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)16},
      UT           = {WOS:000377334000012},
      doi          = {10.1016/j.nuclphysb.2016.03.028},
      url          = {https://bib-pubdb1.desy.de/record/316908},
}