% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@INBOOK{Sigl:410424,
      author       = {Sigl, Guenter},
      title        = {{P}ropagation of {V}ery {H}igh {E}nergy {R}adiation in the
                      {U}niverse},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-03606},
      isbn         = {9783945931219},
      pages        = {379-386},
      year         = {2018},
      comment      = {Sigl, Günter "Propagation of Very High Energy Radiation in
                      the Universe" in Particles, Strings and the Early Universe :
                      The Structure of Matter and Space-Time / Haller, Johannes,
                      Grefe, Michael (eds.), Verlag Deutsches
                      Elektronen-Synchrotron : 2018},
      booktitle     = {Sigl, Günter "Propagation of Very
                       High Energy Radiation in the Universe"
                       in Particles, Strings and the Early
                       Universe : The Structure of Matter and
                       Space-Time / Haller, Johannes, Grefe,
                       Michael (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2018},
      abstract     = {The sources of cosmic rays, in particular ultra-high energy
                      cosmic rays with macroscopic energies above
                      $\sim10^{18}\,$eV, have still not been identified. This is
                      partly caused by the fact that the sky observed in these
                      cosmic rays is surprisingly isotropic and that deflection in
                      galactic and extragalactic magnetic fields may still be
                      substantial. The main goal of project C8 of the SFB 676 was
                      to further develop a general software tool, known as
                      CRPropa, which allows to propagate ultra-high energy cosmic
                      rays from the sources to the observer and make predictions
                      for spectrum, mass composition and sky distribution with a
                      given astrophysical scenario for distribution and injection
                      spectra and composition of the sources and the structure of
                      cosmic magnetic fields.},
      cin          = {UNI/TH},
      cid          = {$I:(DE-H253)UNI_TH-20120731$},
      pnm          = {611 - Fundamental Particles and Forces (POF3-611) / DFG
                      project 13245592 - SFB 676: Teilchen, Strings und frühes
                      Universum: Struktur von Materie und Raum-Zeit (13245592)},
      pid          = {G:(DE-HGF)POF3-611 / G:(GEPRIS)13245592},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)7},
      doi          = {10.3204/PUBDB-2018-00782/C8},
      url          = {https://bib-pubdb1.desy.de/record/410424},
}