% 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”.

@INPROCEEDINGS{Henrichs:600513,
      author       = {Henrichs, Jakob and Nelles, Anna and Aguilar Aguilar, J. A.
                      and Allison, P. and Besson, D. Z. and Bishop, A. and Botner,
                      O. and Bouma, S. and Buitink, S. and Castiglioni, W. and
                      Cataldo, M. and Clark, Aubrey and Coleman, A. and Couberly,
                      K. and Dasgupta, P. and De Kockere, S. and De Vries, Maikel
                      and Deaconu, C. and DuVernois, M. A. and Eimer, A. and
                      Glaser, C. and Gluesenkamp, T. and Hallgren, A. and
                      Hallmann, S. and Hanson, J. C. and Hendricks, B. and
                      Henrichs, J. and Heyer, N. and Hornhuber, C. and Hughes, K.
                      and Karg, T. and Karle, A. and Kelley, John and Korntheuer,
                      M. and Kowalski, M. and Kravchenko, I. and Krebs, R. and
                      Lahmann, R. and Lehmann, P. and Latif, U. A. and Laub, P.
                      and Liu, H. and Mammo, J. and Marsee, M. J. and Meyers,
                      Zachary Samuel and Mikhailova, M. and Michaels, K. and
                      Mulrey, K. and Muzio, M. and Nelles, A. and Novikov, A. and
                      Nozdrina, A. and Oberla, E. and Oeyen, B. and Plaisier, I.
                      and Punsuebsay, N. and Pyras, L. and Ryckbosch, D. and
                      Schlüter, F. and Scholten, O. and Seckel, D. and Seikh, M.
                      F. H. and Smith, D. J. B. and Stoffels, J. and Southall, D.
                      and Terveer, K. and Toscano, S. and Tosi, D. and Van Den
                      Broeck, D. J. and van Eijndhoven, N. and Vieregg, A. G. and
                      Vischer, Janna and Welling, C. and Williams, D. R. and
                      Wissel, S. A. and Young, R. and Zink, A.},
      collaboration = {RNO-{G Collaboration}},
      title        = {{S}earching for cosmic-ray air showers with {RNO}-{G}},
      journal      = {Proceedings of Science / International School for Advanced
                      Studies},
      volume       = {(ICRC2023)},
      issn         = {1824-8039},
      address      = {Trieste},
      publisher    = {SISSA},
      reportid     = {PUBDB-2023-08026},
      series       = {2680794},
      pages        = {259},
      year         = {2023},
      note         = {Pre-published},
      abstract     = {The Radio Neutrino Observatory – Greenland (RNO-G) is an
                      in-iceneutrino detector currently under construction. The
                      detector is designed to make the first measurement of
                      neutrinos beyond energies of $\sim$10 PeV.Each of the
                      planned 35 stations of the detector includes
                      threelog-periodic dipole array antennas (LPDA) pointing
                      towards the sky. The stations cover an area of $\sim$ 50
                      km$^2$ and enable RNO-G to measure the radio emission of
                      cosmic-ray induced air-showers, thus making it a cosmic-ray
                      detector as well. As other experiments have shown, such
                      radio emission can be used to make precision cosmic-ray
                      measurements. Additionally,the location of the experiment at
                      Summit Station, at a height of $\sim$3000 m, enables RNO-G
                      to study the phenomena of shower cores hitting the air/ice
                      boundary and further developing in the ice itself. Moreover,
                      RNO-G is also able to study high energetic muons, created in
                      cosmic-ray induced air-showers, which penetrate into the ice
                      from above. In this contribution, we will give an overview
                      of the cosmic-ray analysis of RNO-G and report the current
                      status. This includes outlining the method used for
                      identifying the air-shower signals using signal templates,
                      showing thefirst cosmic-ray candidate events and discussing
                      systematic uncertainties.},
      month         = {Jul},
      date          = {2023-07-26},
      organization  = {38th International Cosmic Ray
                       Conference, Nagoya (Japan), 26 Jul 2023
                       - 3 Aug 2023},
      keywords     = {showers: atmosphere (INSPIRE) / radio wave: cosmic
                      radiation (INSPIRE) / cosmic radiation: detector (INSPIRE) /
                      ice (INSPIRE) / air (INSPIRE) / muon (INSPIRE) / observatory
                      (INSPIRE) / dipole (INSPIRE)},
      cin          = {Z-RAD},
      ddc          = {530},
      cid          = {I:(DE-H253)Z-RAD-20210408},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)RNO-G-20230101},
      typ          = {PUB:(DE-HGF)16 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.22323/1.444.0259},
      url          = {https://bib-pubdb1.desy.de/record/600513},
}