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@MASTERSTHESIS{Pyras:456326,
      author       = {Pyras, Lilly},
      othercontributors = {Nelles, Anna Friederike and Franckowiak, Anna},
      title        = {{O}ptimizing the triggering strategy for the detection of
                      cosmic rays with the {R}adio {N}eutrino {O}bservatory
                      {G}reenland ({RNO}-{G})},
      school       = {Humboldt Universität zu Berlin},
      type         = {Masterarbeit},
      reportid     = {PUBDB-2021-01462},
      pages        = {90},
      year         = {2020},
      note         = {Masterarbeit, Humboldt Universität zu Berlin, 2020},
      abstract     = {A promising technique to measure neutrinos above 10 PeV is
                      the detection of radio signals generated by the Askaryan
                      effect. The effect is caused by neutrino-induced particle
                      cascades in dense media e.g. ice. Starting in 2021, RNO-G, a
                      new detector using this technique and containing in-ice
                      detector strings will be deployed in Greenland. One of the
                      main challenges of the data analysis will be distinguishing
                      between a cosmic ray muon and a real neutrino event. By
                      building the detector with surface antennas we can use the
                      established method of radio detection of air showers to
                      identify incoming muons and use these signals as veto
                      mechanism in the neutrino detection. An efficient veto
                      trigger will lend higher confidence in identifying neutrinos
                      and prevent the false positive neutrino detection caused by
                      muons. To obtain an efficient veto, a surface trigger
                      mechanism has to be developed and optimized. The trigger is
                      based on the trace envelope in a frequencyband from 80MHz to
                      180MHz. A coincidence of two channels is requires in order
                      to trigger. One RNO-G station will be sensitive to air
                      showers from 1 × $10^17$ eV on. The expected number of
                      detected cosmic rays is 3.17 ± 1.69 per day and station.
                      The overall veto efficiency on a muon event is 29 $\%.$},
      cin          = {Z-RAD / HUB / ZEU-ICE},
      cid          = {I:(DE-H253)Z-RAD-20210408 / I:(DE-H253)HUB-20140108 /
                      I:(DE-H253)ZEU-ICE-20160806},
      pnm          = {613 - Matter and Radiation from the Universe (POF3-613)},
      pid          = {G:(DE-HGF)POF3-613},
      experiment   = {EXP:(DE-H253)IceCube-20150101},
      typ          = {PUB:(DE-HGF)19},
      doi          = {10.3204/PUBDB-2021-01462},
      url          = {https://bib-pubdb1.desy.de/record/456326},
}