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@INPROCEEDINGS{Troitsky:316735,
      author       = {Troitsky, Sergey},
      title        = {{P}arameters of {A}strophysically {M}otivated {A}xion-like
                      {P}articles},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-00133},
      isbn         = {978-3-935702-43-0},
      series       = {DESY-PROC},
      pages        = {72-76},
      year         = {2015},
      comment      = {Troitsky, Sergey "Parameters of Astrophysically Motivated
                      Axion-like Particles" in Proceedings, 11th Patras Workshop
                      on Axions, WIMPs and WISPs (Axion-WIMP 2015) / Irastorza,
                      Igor G., Redondo, Javier, Carmona, José Manuel, Cebrian,
                      Susana, Dafni, Theopisti, Iguaz, Francisco J., Luzon, Gloria
                      (eds.), Verlag Deutsches Elektronen-Synchrotron : 2015 ;
                      AXION-WIMP 2015 : 11th Patras Workshop on Axions, WIMPs and
                      WISPs, 2015-06-22 - 2015-06-26, Zaragoza},
      booktitle     = {Troitsky, Sergey "Parameters of
                       Astrophysically Motivated Axion-like
                       Particles" in Proceedings, 11th Patras
                       Workshop on Axions, WIMPs and WISPs
                       (Axion-WIMP 2015) / Irastorza, Igor G.,
                       Redondo, Javier, Carmona, José Manuel,
                       Cebrian, Susana, Dafni, Theopisti,
                       Iguaz, Francisco J., Luzon, Gloria
                       (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2015 ;
                       AXION-WIMP 2015 : 11th Patras Workshop
                       on Axions, WIMPs and WISPs, 2015-06-22
                       - 2015-06-26, Zaragoza},
      abstract     = {Popular explanations of the anomalous transparency of the
                      Universe for energetic gamma rays include conversion of
                      photons into hypothetical axion-like particles (ALPs) and
                      back in astrophysical magnetic fields. $\J{This$ could
                      either } happen in the gamma-ray source and in the Milky
                      Way, or the photon-ALP oscillations could take place in the
                      intergalactic magnetic fields all along the way between the
                      source and the observer. Given recent astrophysical
                      constraints on ALPs and on intergalactic magnetic fields,
                      these two mechanisms imply very different ALP parameters:
                      masses and couplings. Therefore, confirmation of the
                      anomalies and identification of one of the scenarios would
                      mean cornering of ALP parameters to a particular narrow
                      region.},
      month         = {Jun},
      date          = {2015-06-22},
      organization  = {11th Patras Workshop on Axions, WIMPs
                       and WISPs, Zaragoza (Spain), 22 Jun
                       2015 - 26 Jun 2015},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2015-02/troitsky_sergey},
      url          = {https://bib-pubdb1.desy.de/record/316735},
}