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@INPROCEEDINGS{Gustafsson:408363,
      author       = {Gustafsson, M.},
      collaboration = {Fermi {LAT Collaboration}},
      title        = {{F}ermi-{LAT} and the {G}amma-{R}ay {L}ine {S}earch},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02816, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {215-222},
      year         = {2013},
      comment      = {Gustafsson, M. "Fermi-LAT and the Gamma-Ray Line Search" in
                      Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs
                      (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.),
                      2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions,
                      WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz},
      booktitle     = {Gustafsson, M. "Fermi-LAT and the
                       Gamma-Ray Line Search" in Proceedings,
                       9th Patras Workshop on Axions, WIMPs
                       and WISPs (AXION-WIMP 2013) / Oberlack,
                       Uwe, Sissol, Pierre (eds.), 2013 ;
                       AXION-WIMP 2013 : 9th Patras Workshop
                       on Axions, WIMPs and WISPs , 2013-06-23
                       - 2013-06-28, Mainz},
      abstract     = {A distinct signature for dark matter in the form of weakly
                      interacting massive particles (WIMPs) would be the detection
                      of a monochromatic spectral line in the gamma-ray sky. The
                      Fermi-LAT collaboration has searched for such a line in the
                      energy range from 5 to 300 GeV in five sky regions around
                      the Galactic centre. No globally significant line is
                      detected, and $95\%$ CL upper limits on monochromatic-line
                      strengths are presented. The smallest search region reveals
                      a line-like structure at 133 GeV with a local significance
                      of 2.9 σ after 4.4 years of data, which translates to less
                      than 1σ global significance from a trial factor of around
                      200.},
      month         = {Jun},
      date          = {2013-06-24},
      organization  = {9th Patras Workshop on Axions, WIMPs
                       and WISPs, Mainz (Germany), 24 Jun 2013
                       - 28 Jun 2013},
      keywords     = {Hypothetisches Teilchen (gnd)},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2013-04/gustafsson_michael},
      url          = {https://bib-pubdb1.desy.de/record/408363},
}