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@ARTICLE{Joffre:618904,
      author       = {Joffre, Scott D. and Torres-Albà, Núria and Ajello, Marco
                      and Kocevski, Daniel and Bühler, Rolf},
      title        = {{H}istorical {F}ermi {A}ll-sky {V}ariability {A}nalysis of
                      {G}alactic {F}lares},
      journal      = {The astrophysical journal / Part 1},
      volume       = {968},
      number       = {1},
      issn         = {0004-637X},
      address      = {London},
      publisher    = {Institute of Physics Publ.},
      reportid     = {PUBDB-2024-07226, arXiv:2402.07994},
      pages        = {44},
      year         = {2024},
      note         = {Submitted to ApJ Feb. 28 2024. Minor edits in Section 4 and
                      5 for clarity. 26 pages, 6 figures, 5 Tables},
      abstract     = {The Fermi All-sky Variability Analysis (FAVA) provides a
                      photometric alternative for identifying week-long gamma-ray
                      flares across the entire sky while being independent of any
                      diffuse Galactic or isotropic emission model. We reviewed
                      779 weeks of Fermi Large Area Telescope data analyzed by
                      FAVA to estimate the rate and origin of Galactic gamma-ray
                      flares, and to search for new variable Galactic gamma-ray
                      transients. We report an estimated yearly rate of ∼8.5
                      Galactic gamma-ray flares yr$^{–1}$, with ∼1 flare
                      yr$^{–1}$ coming from unknown sources. Out of the known
                      gamma-ray sources that are spatially coincident with these
                      detected flares, we report gamma-ray flares for six of them
                      for the first time. All six are classified as pulsars, or a
                      source of unknown nature but which positionally overlaps
                      with known supernova remnants or pulsar wind nebulae (PWNe).
                      This potentially means these sites are tentative candidates
                      to be the second known site of a variable gamma-ray PWN,
                      after the famous Crab Nebula’s PWN. Additionally, we
                      identify nine unassociated flares that are unlikely to have
                      originated from known gamma-ray sources.},
      cin          = {$Z_GA$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_GA-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)TAIGA-20190101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2402.07994},
      howpublished = {arXiv:2402.07994},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2402.07994;\%\%$},
      UT           = {WOS:001248939900001},
      doi          = {10.3847/1538-4357/ad4494},
      url          = {https://bib-pubdb1.desy.de/record/618904},
}