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@ARTICLE{Aleksi:207275,
      author       = {Aleksić, J. and Ansoldi, S. and Antonelli, L. A. and
                      Antoranz, P. and Babic, A. and Bangale, P. and Barrio, J. A.
                      and González, J. Becerra and Bednarek, W. and Bernardini,
                      E. and Biasuzzi, B. and Biland, A. and Blanch, O. and
                      Bonnefoy, S. and Bonnoli, G. and Borracci, F. and Bretz, T.
                      and Carmona, E. and Carosi, A. and Colin, P. and Colombo, E.
                      and Contreras, J. L. and Cortina, J. and Covino, S. and Da
                      Vela, P. and Dazzi, F. and De Angelis, A. and De Caneva, G.
                      and De Lotto, B. and Wilhelmi, E. de Oña and Mendez, C.
                      Delgado and Prester, D. Dominis and Dorner, D. and Doro, M.
                      and Einecke, S. and Eisenacher, D. and Elsaesser, D. and
                      Fidalgo, D. and Fonseca, M. V. and Font, L. and Frantzen, K.
                      and Fruck, C. and Galindo, D. and López, R. J. García and
                      Garczarczyk, M. and Terrats, D. Garrido and Gaug, M. and
                      Godinović, N. and Muñoz, A. González and Gozzini, S. R.
                      and Hadasch, D. and Hanabata, Y. and Hayashida, M. and
                      Herrera, J. and Hildebrand, D. and Hose, J. and Hrupec, D.
                      and Idec, W. and Kadenius, V. and Kellermann, H. and
                      Knoetig, M. L. and Kodani, K. and Konno, Y. and Krause, J.
                      and Kubo, H. and Kushida, J. and La Barbera, A. and Lelas,
                      D. and Lewandowska, N. and Lindfors, E. and Lombardi, S. and
                      Longo, F. and López, M. and López-Coto, R. and
                      López-Oramas, A. and Lorenz, E. and Lozano, I. and
                      Makariev, M. and Mallot, K. and Maneva, G. and Mankuzhiyil,
                      N. and Mannheim, K. and Maraschi, L. and Marcote, B. and
                      Mariotti, M. and Martínez, M. and Mazin, D. and Menzel, U.
                      and Miranda, J. M. and Mirzoyan, R. and Moralejo, A. and
                      Munar-Adrover, P. and Nakajima, D. and Neustroev, V. and
                      Niedzwiecki, A. and Nilsson, K. and Nishijima, K. and Noda,
                      K. and Orito, R. and Overkemping, A. and Paiano, S. and
                      Palatiello, M. and Paneque, D. and Paoletti, R. and Paredes,
                      J. M. and Paredes-Fortuny, X. and Persic, M. and Poutanen,
                      J. and Moroni, P. G. Prada and Prandini, E. and Puljak, I.
                      and Reinthal, R. and Rhode, W. and Ribó, M. and Rico, J.
                      and Garcia, J. Rodriguez and Rügamer, S. and Saito, T. and
                      Saito, K. and Satalecka, K. and Scalzotto, V. and Scapin, V.
                      and Schultz, C. and Schweizer, T. and Shore, S. N. and
                      Sillanpää, A. and Sitarek, J. and Snidaric, I. and
                      Sobczynska, D. and Spanier, F. and Stamerra, A. and
                      Steinbring, T. and Storz, J. and Strzys, M. and Takalo, L.
                      and Takami, H. and Tavecchio, F. and Temnikov, P. and
                      Terzić, T. and Tescaro, D. and Teshima, M. and Thaele, J.
                      and Tibolla, O. and Torres, D. F. and Toyama, T. and Treves,
                      A. and Vogler, P. and Will, M. and Zanin, R.},
      title        = {{M}easurement of the {C}rab {N}ebula {S}pectrum over
                      {T}hree {D}ecades in {E}nergy with the {MAGIC} {T}elescopes},
      reportid     = {PUBDB-2015-01258, arXiv:1406.6892},
      year         = {2014},
      note         = {OA},
      abstract     = {The MAGIC stereoscopic system collected 69 hours of Crab
                      Nebula data between October 2009 and April 2011. Analysis of
                      this data sample using the latest improvements in the MAGIC
                      stereoscopic software provided an unprecedented precision of
                      spectral and night-by-night light curve determination at
                      gamma rays. We derived a differential spectrum with a single
                      instrument from 50 GeV up to almost 30 TeV with 5 bins per
                      energy decade. In the low energies, MAGIC results, combined
                      with the Fermi-LAT data, show a flat Inverse Compton peak.
                      The Fermi-LAT and MAGIC spectral data were fit from 1 GeV to
                      30 TeV with a log-parabola, yielding a peak position at (53
                      $\pm$ 3) GeV with a $\chi^2_{red}$ = 82/27 (error probably
                      underestimated due to the bad fit quality), showing that the
                      log-parabola is not a good representation of the Inverse
                      Compton peak of the Crab Nebula. There is no hint of the
                      integral flux variability on daily scales at energies above
                      300 GeV if accounting for systematic uncertainties of the
                      measurement. We consider two state-of-the-art theoretical
                      models to describe the overall spectral energy distribution
                      of the Crab Nebula. The constant B-field model cannot
                      satisfactorily reproduce the VHE spectral measurements
                      presented in this work, mostly troubled by the broadness of
                      the observed IC peak. Most probably this implies that the
                      assumption of the homogeneity of the magnetic field inside
                      the nebula is incorrect. On the other hand, the
                      time-dependent 1D spectral model provides a good fit of the
                      new VHE results when considering a 80 {\mu}G magnetic field.
                      However, it fails to match the data when including the
                      morphology of the nebula at lower wavelengths.},
      cin          = {ZEU-EXP/AT},
      cid          = {$I:(DE-H253)ZEU-EXP_AT-20120731$},
      pnm          = {523 - High-energy gamma ray astronomy (POF2-523)},
      pid          = {G:(DE-HGF)POF2-523},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)25 / PUB:(DE-HGF)15},
      eprint       = {1406.6892},
      howpublished = {arXiv:1406.6892},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:1406.6892;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/207275},
}