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@ARTICLE{Aliu:156860,
      author       = {Aliu, E. and Archambault, S. and Arlen, T. and Aune, T. and
                      Beilicke, M. and Benbow, W. and Bird, R. and Böttcher, M.
                      and Bouvier, A. and Bugaev, V. and Byrum, K. and Cesarini,
                      A. and Ciupik, L. and Collins-Hughes, E. and Connolly, M. P.
                      and Cui, W. and Dickherber, R. and Duke, C. and Dumm, J. and
                      Errando, M. and Falcone, A. and Federici, Simone and Feng,
                      Q. and Finley, J. P. and Finnegan, G. and Fortson, L. and
                      Furniss, A. and Galante, N. and Gall, D. and Gillanders, G.
                      H. and Griffin, S. and Grube, J. and Gyuk, G. and Hanna, D.
                      and Holder, J. and Hughes, G. and Humensky, T. B. and
                      Kaaret, P. and Kertzman, M. and Khassen, Y. and Kieda, D.
                      and Krawczynski, H. and Krennrich, F. and Lang, M. J. and
                      Madhavan, A. S and Maier, G. and Majumdar, P. and McArthur,
                      S. and McCann, A. and Moriarty, P. and Mukherjee, R. and
                      Nelson, T. and O'Faoláin de Bhróithe, A. and Ong, R. A.
                      and Orr, M. and Otte, A. N. and Park, N. and Perkins, J. S.
                      and Pichel, A. and Pohl, Martin and Popkow, A. and Prokoph,
                      H. and Quinn, J. and Ragan, K. and Reyes, L. C. and
                      Reynolds, P. T. and Roache, E. and Saxon, D. B. and
                      Schroedter, M. and Sembroski, G. H. and Skole, C. and Smith,
                      A. W. and Staszak, D. and Telezhinsky, I. and Theiling, M.
                      and Tyler, J. and Varlotta, A. and Vassiliev, V. V. and
                      Wakely, S. P. and Weekes, T. C. and Weinstein, A. and
                      Welsing, R. and Williams, D. A. and Zitzer, B.},
      title        = {{MULTIWAVELENGTH} {OBSERVATIONS} {AND} {MODELING} {OF}
                      1{ES} 1959+650 {IN} {A} {LOW} {FLUX} {STATE}},
      journal      = {The astrophysical journal},
      volume       = {775},
      number       = {1},
      issn         = {1538-4357},
      address      = {Chicago, Ill. [u.a.]},
      publisher    = {Univ.11032},
      reportid     = {DESY-2014-00171},
      pages        = {3},
      year         = {2013},
      abstract     = {We report on the VERITAS observations of the high-frequency
                      peaked BL Lac object 1ES 1959+650 in the period 2007-2011.
                      This source is detected at TeV energies by VERITAS at 16.4
                      standard deviation (σ) significance in 7.6 hr of
                      observation in a low flux state. A multiwavelength spectral
                      energy distribution (SED) is constructed from
                      contemporaneous data from VERITAS, Fermi-LAT, RXTE PCA, and
                      Swift UVOT. Swift XRT data is not included in the SED due to
                      a lack of simultaneous observations with VERITAS. In
                      contrast to the orphan γ-ray flare exhibited by this source
                      in 2002, the X-ray flux of the source is found to vary by an
                      order of magnitude, while other energy regimes exhibit less
                      variable emission. A quasi-equilibrium synchrotron
                      self-Compton model with an additional external radiation
                      field is used to describe three SEDs corresponding to the
                      lowest, highest, and average X-ray states. The variation in
                      the X-ray spectrum is modeled by changing the electron
                      injection spectral index, with minor adjustments of the
                      kinetic luminosity in electrons. This scenario produces
                      small-scale flux variability of the order of lsim 2 in the
                      high energy (E > 1 MeV) and very high energy (E > 100 GeV)
                      γ-ray regimes, which is corroborated by the Fermi-LAT,
                      VERITAS, and Whipple 10 m telescope light curves.},
      cin          = {$Z_THAT$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_THAT-20210408$},
      pnm          = {52x - Programm Astroteilchenphysik - Topic unbekannt
                      (POF2-52x)},
      pid          = {G:(DE-HGF)POF2-52x},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)16},
      UT           = {WOS:000324615800003},
      doi          = {10.1088/0004-637X/775/1/3},
      url          = {https://bib-pubdb1.desy.de/record/156860},
}