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@PROCEEDINGS{Caballero:296846,
      key          = {296846},
      editor       = {Caballero, Rogelio and D'Olivo, Juan Carlos and
                      Medina-Tanco, Gustavo and Nellen, Lukas and Sánchez,
                      Federico A. and Valdés-Galicia, José F.},
      title        = {{P}roceedings, 30th {I}nternational {C}osmic {R}ay
                      {C}onference ({ICRC} 2007)},
      address      = {Ciudad de Mexico},
      publisher    = {Universidad Nacional Autonoma de Mexico},
      reportid     = {PUBDB-2016-01641, arXiv:0711.0353},
      year         = {2007},
      abstract     = {This paper bundles 40 contributions by the IceCube
                      collaboration that were submitted to the 30th International
                      Cosmic Ray Conference ICRC 2007. The articles cover studies
                      on cosmic rays and atmospheric neutrinos, searches for
                      non-localized, extraterrestrial electron, muon and tau
                      neutrino signals, scans for steady and intermittent neutrino
                      point sources, searches for dark matter candidates, magnetic
                      monopoles and other exotic particles, improvements in
                      analysis techniques, as well as future detector extensions.
                      The IceCube observatory will be finalized in 2011 to form a
                      cubic-kilometer ice-Cherenkov detector at the location of
                      the geographic South Pole. At the present state of
                      construction, IceCube consists of 52 paired IceTop surface
                      tanks and 22 IceCube strings with a total of 1426 Digital
                      Optical Modules deployed at depths up to 2350 m. The
                      observatory also integrates the 19 string AMANDA
                      subdetector, that was completed in 2000 and extends
                      IceCube's reach to lower energies. Before the deployment of
                      IceTop, cosmic air showers were registered with the 30
                      station SPASE-2 surface array. IceCube's low noise Digital
                      Optical Modules are very reliable, show a uniform response
                      and record waveforms of arriving photons that are resolvable
                      with nanosecond precision over a large dynamic range. Data
                      acquisition, reconstruction and simulation software are
                      running in production mode and the analyses, profiting from
                      the improved data quality and increased overall sensitivity,
                      are well under way.},
      month         = {Jul},
      date          = {2007-07-03},
      organization  = {30th International Cosmic Ray
                       Conference, Merida (Mexico), 3 Jul 2007
                       - 11 Jul 2007},
      cin          = {ZNP(-2012)},
      cid          = {$I:(DE-H253)ZNP_-2012_-20130307$},
      pnm          = {520 - Astroteilchenphysik (POF1-500)},
      pid          = {G:(DE-HGF)POF1-520},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)26 / PUB:(DE-HGF)29},
      eprint       = {0711.0353},
      howpublished = {arXiv:0711.0353},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:0711.0353;\%\%$},
      url          = {https://bib-pubdb1.desy.de/record/296846},
}