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Abstract
The Radio Neutrino Observatory Greenland (RNO-G) is planned to be the first large-scale implementation of the in-ice radio detection technique. It targets astrophysical as well as cosmogenic neutrinos with energies above 10 PeV. The deep component of a single RNO-G station consists of three strings with antennas to capture horizontal as well as vertical polarization. This contribution shows a model-based approach to reconstruct the direction of the neutrinos with an RNO-G station. The timing of the waveforms is used to reconstruct the vertex position and the shape and amplitude of the waveform are used to reconstruct the viewing angle as well as the polarization, which will add up to the zenith and azimuth direction of the neutrino. We present the achieved angular resolution and discuss implications for the science of RNO-G.

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MLA
Plaisier, Ilse, et al. “Direction Reconstruction for the Radio Neutrino Observatory Greenland.” Proceedings of 37th International Cosmic Ray Conference (ICRC2021), vol. 395, 2021, doi:10.22323/1.395.1026.
APA
Plaisier, I., Aguilar, J. A., Allison, P., Beatty, J. J., Bernhoff, H., Besson, D. Z., … Rno-g, [missing]. (2021). Direction reconstruction for the Radio Neutrino Observatory Greenland. Proceedings of 37th International Cosmic Ray Conference (ICRC2021), 395. https://doi.org/10.22323/1.395.1026
Chicago author-date
Plaisier, Ilse, Juan A. Aguilar, Patrick Allison, James J. Beatty, Hans Bernhoff, David Zeke Besson, Nils Bingefors, et al. 2021. “Direction Reconstruction for the Radio Neutrino Observatory Greenland.” In Proceedings of 37th International Cosmic Ray Conference (ICRC2021). Vol. 395. https://doi.org/10.22323/1.395.1026.
Chicago author-date (all authors)
Plaisier, Ilse, Juan A. Aguilar, Patrick Allison, James J. Beatty, Hans Bernhoff, David Zeke Besson, Nils Bingefors, Olga Botner, Sjoerd Bouma, Stijn Buitink, Katie Carter, Maddalena Cataldo, Brian A. Clark, Zachary Curtis-Ginsberg, Amy L. Connolly, Paramita Dasgupta, Simon De Kockere, Krijn D. de Vries, Cosmin Deaconu, Michael A. DuVernois, Christian Glaser, Allan Hallgren, Steffen Hallmann, Jordan C. Hanson, Bryan Hendricks, Benjamin Hokanson-Fasig, Christian Hornhuber, Kaeli Hughes, Albrecht Karle, John L. Kelley, Spencer R. Klein, Ryan Krebs, Robert Lahmann, Uzair Abdul Latif, Mitchell Magnuson, Thomas Meures, Zachary S. Meyers, Katharine Mulrey, Anna Nelles, Alexander Novikov, Eric Oberla, Bob Oeyen, Hershal Pandya, Lilly Pyras, Dirk Ryckbosch, Olaf Scholten, David Seckel, Daniel Smith, Daniel Southall, Jorge Torres, Simona Toscano, Delia Tosi, Dieder J. Van Den Broeck, Nick van Eijndhoven, Abigail G. Vieregg, Christoph Welling, Stephanie Wissel, Robert Young, Adrian Zink, and [missing] Rno-g. 2021. “Direction Reconstruction for the Radio Neutrino Observatory Greenland.” In Proceedings of 37th International Cosmic Ray Conference (ICRC2021). Vol. 395. doi:10.22323/1.395.1026.
Vancouver
1.
Plaisier I, Aguilar JA, Allison P, Beatty JJ, Bernhoff H, Besson DZ, et al. Direction reconstruction for the Radio Neutrino Observatory Greenland. In: Proceedings of 37th International Cosmic Ray Conference (ICRC2021). 2021.
IEEE
[1]
I. Plaisier et al., “Direction reconstruction for the Radio Neutrino Observatory Greenland,” in Proceedings of 37th International Cosmic Ray Conference (ICRC2021), Online, 2021, vol. 395.
@inproceedings{8716297,
  abstract     = {{The Radio Neutrino Observatory Greenland (RNO-G) is planned to be the first large-scale implementation of the in-ice radio detection technique. It targets astrophysical as well as cosmogenic neutrinos with energies above 10 PeV. The deep component of a single RNO-G station consists of three strings with antennas to capture horizontal as well as vertical polarization. This contribution shows a model-based approach to reconstruct the direction of the neutrinos with an RNO-G station. The timing of the waveforms is used to reconstruct the vertex position and the shape and amplitude of the waveform are used to reconstruct the viewing angle as well as the polarization, which will add up to the zenith and azimuth direction of the neutrino. We present the achieved angular resolution and discuss implications for the science of RNO-G.}},
  author       = {{Plaisier, Ilse and Aguilar, Juan A. and Allison, Patrick and Beatty, James J. and Bernhoff, Hans and Besson, David Zeke and Bingefors, Nils and Botner, Olga and Bouma, Sjoerd and Buitink, Stijn and Carter, Katie and Cataldo, Maddalena and Clark, Brian A. and Curtis-Ginsberg, Zachary and Connolly, Amy L. and Dasgupta, Paramita and De Kockere, Simon and de Vries, Krijn D. and Deaconu, Cosmin and DuVernois, Michael A. and Glaser, Christian and Hallgren, Allan and Hallmann, Steffen and Hanson, Jordan C. and Hendricks, Bryan and Hokanson-Fasig, Benjamin and Hornhuber, Christian and Hughes, Kaeli and Karle, Albrecht and Kelley, John L. and Klein, Spencer R. and Krebs, Ryan and Lahmann, Robert and Latif, Uzair Abdul and Magnuson, Mitchell and Meures, Thomas and Meyers, Zachary S. and Mulrey, Katharine and Nelles, Anna and Novikov, Alexander and Oberla, Eric and Oeyen, Bob and Pandya, Hershal and Pyras, Lilly and Ryckbosch, Dirk and Scholten, Olaf and Seckel, David and Smith, Daniel and Southall, Daniel and Torres, Jorge and Toscano, Simona and Tosi, Delia and Van Den Broeck, Dieder J. and van Eijndhoven, Nick and Vieregg, Abigail G. and Welling, Christoph and Wissel, Stephanie and Young, Robert and Zink, Adrian and Rno-g, [missing]}},
  booktitle    = {{Proceedings of 37th International Cosmic Ray Conference (ICRC2021)}},
  issn         = {{1824-8039}},
  language     = {{eng}},
  location     = {{Online}},
  title        = {{Direction reconstruction for the Radio Neutrino Observatory Greenland}},
  url          = {{http://doi.org/10.22323/1.395.1026}},
  volume       = {{395}},
  year         = {{2021}},
}

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