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@ARTICLE{Abramowski:293214,
      author       = {Abramowski, A. and Aharonian, F. and Benkhali, F. Ait and
                      Akhperjanian, A. G. and Angüner, E. O. and Backes, M. and
                      Balenderan, S. and Balzer, A. and Barnacka, A. and
                      Becherini, Y. and Tjus, J. Becker and Berge, D. and
                      Bernhard, S. and Bernlöhr, K. and Birsin, E. and Biteau, J.
                      and Böttcher, M. and Boisson, C. and Bolmont, J. and
                      Bordas, P. and Bregeon, J. and Brun, F. and Brun, P. and
                      Bryan, M. and Bulik, T. and Carrigan, S. and Casanova, S.
                      and Chadwick, P. M. and Chakraborty, N. and Chalme-Calvet,
                      R. and Chaves, R. C. G. and Chrétien, M. and Colafrancesco,
                      S. and Cologna, G. and Conrad, J. and Couturier, C. and Cui,
                      Y. and Dalton, M. and Davids, I. D. and Degrange, B. and
                      Deil, C. and deWilt, P. and Djannati-Ataï, A. and Domainko,
                      W. and Donath, A. and Drury, L. O’C. and Dubus, G. and
                      Dutson, K. and Dyks, J. and Dyrda, M. and Edwards, T. and
                      Egberts, K. and Eger, P. and Espigat, P. and Farnier, C. and
                      Fegan, S. and Feinstein, F. and Fernandes, M. V. and
                      Fernandez, D. and Fiaßon, A. and Fontaine, G. and Förster,
                      A. and FüSSling, M. and Gabici, S. and Gajdus, M. and
                      Gallant, Y. A. and Garrigoux, T. and Giavitto, G. and
                      Giebels, B. and Glicenstein, J. F. and Gottschall, D. and
                      Grondin, M.-H. and Grudzińska, M. and Hadsch, D. and
                      Häffner, S. and Hahn, J. and Harris, J. and Heinzelmann, G.
                      and Henri, G. and Hermann, G. and Hervet, O. and Hillert, A.
                      and Hinton, J. A. and Hofmann, W. and Hofverberg, P. and
                      Holler, M. and Horns, D. and Ivascenko, A. and Jacholkowska,
                      A. and Jahn, C. and Jamrozy, M. and Janiak, M. and
                      Jankowsky, F. and Jung, I. and Kastendieck, M. A. and
                      Katarzyński, K. and Katz, U. and Kaufmann, S. and Khélifi,
                      B. and Kieffer, M. and Klepser, S. and Klochkov, D. and
                      Kluźniak, W. and Kolitzus, D. and Komin, Nu. and Kosack, K.
                      and Krakau, S. and Krayzel, F. and Krüger, P. P. and
                      Laffon, H. and Lamanna, G. and Lefaucheur, J. and Lefranc,
                      V. and Lemiére, A. and Lemoine-Goumard, M. and Lenain,
                      J.-P. and Lohse, T. and Lopatin, A. and Lu, C.-C. and
                      Marandon, V. and Marcowith, A. and Marx, R. and Maurin, G.
                      and Maxted, N. and Mayer, M. and McComb, T. J. L. and
                      Méhault, J. and Meintjes, P. J. and Menzler, U. and Meyer,
                      M. and Mitchell, A. M. W. and Moderski, R. and Mohamed, M.
                      and Morå, K. and Moulin, E. and Murach, T. and Naurois, M.
                      de and Niemiec, J. and Nolan, S. J. and Oakes, L. and Odaka,
                      H. and Ohm, S. and Opitz, B. and Ostrowski, M. and Oya, I.
                      and Panter, M. and Parsons, R. D. and Paz Arribas, M. and
                      Pekeur, N. W. and Pelletier, G. and Perez, J. and Petrucci,
                      P.-O. and Peyaud, B. and Pita, S. and Poon, H. and
                      Pühlhofer, G. and Punch, M. and Quirrenbach, A. and Raab,
                      S. and Reichardt, I. and Reimer, A. and Reimer, O. and
                      Renaud, M. and de los Reyes, R. and Rieger, F. and Rob, L.
                      and Romoli, C. and Rosier-Lees, S. and Rowell, G. and Rudak,
                      B. and Rulten, C. B. and Sahakian, V. and Salek, D. and
                      Sanchez, D. A. and Santangelo, A. and Schlickeiser, R. and
                      Schüssler, F. and Schulz, A. and Schwanke, U. and
                      Schwarzburg, S. and Schwemmer, S. and Sol, H. and Spanier,
                      F. and Spengler, G. and Spies, F. and Stawarz, Ł. and
                      Steenkamp, R. and Stegmann, C. and Stinzing, F. and Stycz,
                      K. and Sushch, I. and Tavernet, J.-P. and Tavernier, T. and
                      Taylor, A. M. and Terrier, R. and Tluczykont, M. and
                      Trichard, C. and Valerius, K. and van Eldik, C. and van
                      Soelen, B. and Vasileiadis, G. and Veh, J. and Venter, C.
                      and Viana, A. and Vincent, P. and Vink, J. and Völk, H. J.
                      and Volpe, F. and Vorster, M. and Vuillaume, T. and Wagner,
                      P. and Wagner, R. M. and Ward, M. and Weidinger, M. and
                      Weitzel, Q. and White, R. and Wierzcholska, A. and Willmann,
                      P. and Wörnlein, A. and Wouters, D. and Yang, R. and
                      Zabalza, V. and Zaborov, D. and Zacharias, M. and Zdziarski,
                      A. A. and Zech, A. and Zechlin, H.-S.},
      collaboration = {H.E.S.S.{ Collaboration}},
      title        = {{T}he 2012 {F}lare of {PG} 1553+113 {S}een with
                      {H}.{E}.{S}.{S}. and {F}ermi -{L}at},
      journal      = {The astrophysical journal / 1},
      volume       = {802},
      number       = {1},
      issn         = {1538-4357},
      address      = {Chicago, Ill. [u.a.]},
      publisher    = {Univ.11032},
      reportid     = {PUBDB-2016-00370},
      pages        = {65 -},
      year         = {2015},
      note         = {(c) The American Astronomical Society},
      abstract     = {Very high energy (VHE, E > 100 GeV) $\gamma-ray$ flaring
                      activity of the high-frequency peaked BL Lac object PG
                      1553+113 has been detected by the H.E.S.S. telescopes. The
                      flux of the source increased by a factor of 3 during the
                      nights of 2012 April 26 and 27 with respect to the archival
                      measurements with a hint of intra-night variability. No
                      counterpart of this event has been detected in the
                      Fermi-Large Area Telescope data. This pattern is consistent
                      with VHE $\gamma-ray$ flaring being caused by the injection
                      of ultrarelativistic particles, emitting $\gamma-rays$ at
                      the highest energies. The dataset offers a unique
                      opportunity to constrain the redshift of this source at z =
                      0.49 $\pm$ 0.04 using a novel method based on Bayesian
                      statistics. The indication of intra-night variability is
                      used to introduce a novel method to probe for a possible
                      Lorentz invariance violation (LIV), and to set limits on the
                      energy scale at which Quantum Gravity (QG) effects causing
                      LIV may arise. For the subluminal case, the derived limits
                      are $E_{QG,1}$ > 4.10 × $10^{17}$ GeV and $E_{QG,2}$ > 2.10
                      × $10^{10}$ GeV for linear and quadratic LIV effects,
                      respectively.},
      cin          = {ZEU-HESS},
      ddc          = {520},
      cid          = {I:(DE-H253)ZEU-HESS-20140213},
      pnm          = {613 - Matter and Radiation from the Universe (POF3-613) /
                      P-WIND - New light on the gamma-ray sky: unveiling
                      cosmic-ray accelerators in the Milky Way and their relation
                      to pulsar wind nebulae (259391)},
      pid          = {G:(DE-HGF)POF3-613 / G:(EU-Grant)259391},
      experiment   = {EXP:(DE-MLZ)External-20140101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000351834700065},
      doi          = {10.1088/0004-637X/802/1/65},
      url          = {https://bib-pubdb1.desy.de/record/293214},
}