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@INPROCEEDINGS{Tluczykont:315086,
      author       = {Tluczykont, Martin and Budnev, N. and Astapov, I. and
                      Bezyazeekov, P. and Bogdanov, A. and Boreyko, V. and
                      Brueckner, Martin and Chiavassa, A. and Chvalaev, O. and
                      Gress, O. and Gress, T. and Grishin, O. and Dyachok, A. and
                      Epimakhov, Sergey and Fedorov, O. and Gafarov, A. and
                      Gorbunov, N. and Grebenyuk, V. and Grinuk, A. and Horns,
                      Dieter and Ivanova, Anna and Kalinin, Anton and Karpov, N.
                      and Kalmykov, N. and Kazarina, Y. and Kirichkov, N. and
                      Kiryuhin, S. and Kokoulin, R. and Komponiest, K. and
                      Konstantinov, A. and Korosteleva, E. and Kozhin, V. and
                      Kunnas, Maike Helena and Kuzmichev, L. and Lenok, V. and
                      Lubsandorzhiev, B. and Lubsandorzhiev, N. and Mirgazov, R.
                      and Mirzoyan, R. and Monkhoev, R. and Nachtigall, Rayk and
                      Osipova, E. and Pakhorukov, A. and Panasyuk, M. and Pankov,
                      L. and Petrukhin, A. and Platonov, V. and Poleschuk, V. and
                      Popova, Elena and Porelli, Andrea and Postnikov, E. and
                      Prosin, V. and Ptuskin, V. and Rubtsov, G. and Pushnin, A.
                      and Samoliga, V. and Satunin, Peter and Semeney, Yu. and
                      Silaev, A. and Silaev, A. and Skurikhin, A. and Slucka, V.
                      and Spiering, Christian and Sveshnikova, L. and Tabolenko,
                      V. and Tarashansky, B. and Tkachenko, A. and Tkachev, L. and
                      Voronin, D. and Wischnewski, Ralf and Zagorodnikov, A. and
                      Zurbanov, V. and Yashin, I.},
      title        = {{C}onnecting neutrino {A}strophysics to {M}ulti-{T}e{V} to
                      {P}e{V} gamma-ray astronomy with {TAIGA}},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05621},
      isbn         = {978-3-945931-08-0},
      series       = {DESY-PROC},
      pages        = {135-142},
      year         = {2016},
      comment      = {Tluczykont, M. "Connecting neutrino Astrophysics to
                      Multi-TeV to PeV gamma-ray astronomy with TAIGA" in
                      Proceedings, Magellan Workshop: Connecting Neutrino Physics
                      and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko,
                      Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron,
                      DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18,
                      Hamburg},
      booktitle     = {Tluczykont, M. "Connecting neutrino
                       Astrophysics to Multi-TeV to PeV
                       gamma-ray astronomy with TAIGA" in
                       Proceedings, Magellan Workshop:
                       Connecting Neutrino Physics and
                       Astronomy / Dahmke, Stefan K.G., Meyer,
                       Mikko, Vanhoefer, Laura (eds.),
                       Deutsches Elektronen-Synchrotron, DESY
                       : 2016 ; Magellan Workshop, 2016-03-17
                       - 2016-03-18, Hamburg},
      abstract     = {Recent evidence for neutrinos in the PeV energy range from
                      IceCube provides additional motivation for the search for
                      the most energetic Galactic accelerators. Gamma-ray
                      astronomy is a sound strategy to reach this goal, providing
                      the energy range beyond $10\,TeV$ can be covered at a
                      sufficient sensitivity level. The energy spectra of most
                      known gamma-ray emitters only reach up to few 10s of TeV.
                      The HEGRA IACT installation reported evidence for gamma-ray
                      energies from the Crab Nebula as high as $80\,TeV.$
                      Uncovering their spectral shape up to few 100s of TeV could
                      answer the question whether some of these objects are cosmic
                      ray Pevatrons, i.e. Galactic PeV accelerators. Extending
                      observations beyond this energy range requires very large
                      effective detector areas, as planned by the TAIGA
                      collaboration.},
      month         = {Mar},
      date          = {2016-03-17},
      organization  = {Magellan Workshop, Hamburg (Germany),
                       17 Mar 2016 - 18 Mar 2016},
      cin          = {ZEU-EXP/AT / ZEU-ICE},
      cid          = {$I:(DE-H253)ZEU-EXP_AT-20120731$ /
                      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-MLZ)External-20140101},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      UT           = {WOS:00},
      doi          = {10.3204/DESY-PROC-2016-05/27},
      url          = {https://bib-pubdb1.desy.de/record/315086},
}