PoS - Proceedings of Science
Volume 444 - 38th International Cosmic Ray Conference (ICRC2023) - Neutrino Astronomy & Physics (NU)
Status and recent results from the Radio Neutrino Observatory in Greenland (RNO-G)
 RNO-G Collaboration, J. Aguilar, P. Allison, D. Besson, A. Bishop, O. Botner, S. Bouma, S. Buitink, W. Castiglioni, M. Cataldo, B. Clark, A. Coleman, K. Couberly, P. Dasgupta, S. De Kockere, K. de Vries, C. Deaconu, M. DuVernois, A. Eimer, C. Glaser, T. Glüsenkamp, A. Hallgren, S. Hallmann*, J. Hanson, B.L. Hendricks, J. Henrichs, N. Heyer, C. Hornhuber, K. Hughes, T. Karg, A. Karle, J. Kelley, M. Korntheuer, M. Kowalski, I. Kravchenko, R. Krebs, R. Lahmann, P. Lehmann, U.A. Latif, P. Laub, C. Liu, J. Mammo, M. Marsee, Z.S. Meyers, M. Mikhailova, K. Michaels, K. Mulrey, M.S. Muzio, A. Nelles, A. Novikov, A. Nozdrina, E. Oberla, B. Oeyen, I. Plaisier, N. Punsuebsay, L. Pyras, D. Ryckbosch, F. Schlüter, O. Scholten, D. Seckel, M. Seikh, D. Smith, J. Stoffels, D. Southall, K. Terveer, S. Toscano, D. Tosi, D. Van den Broeck, N. van Eijndhoven, A.G. Vieregg, J. Vischer, C. Welling, D. Williams, S. Wissel, R. Young and A. Zinket al. (click to show)
Full text: pdf
Pre-published on: August 18, 2023
Published on: September 27, 2024
Abstract
The Radio Neutrino Observatory in Greenland (RNO-G) is an in-ice radio detector for the detection
of ultra-high energy neutrinos beyond ∼10 PeV. The array is under construction and will consist
of 35 stations, with the potential to make the first detection of a neutrino-induced particle shower
via the Askaryan emission. Stations operate autonomously and consist of both deep antennas
deployed down to -100m in the ice, and high-gain log-periodic dipole antennas buried near the
surface.

In total, seven RNO-G stations were installed during the 2021 and 2022 field seasons and are
collecting data since. Here, we present the current status and performance of the experiment. We
present results from first analyses using the deep and shallow components of the instrument.
DOI: https://doi.org/10.22323/1.444.1043
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