par Aguilar Sanchez, Juan Antonio 
;Schlüter, Felix ;Toscano, Simona ; [et al.]
Référence (26 July 2023 through 3 August 2023: Nagoya), 38th International Cosmic Ray Conference, ICRC 2023, Pos proceedings of science (444), 1043
Publication Publié, 2024-03-01
;Schlüter, Felix ;Toscano, Simona ; [et al.]Référence (26 July 2023 through 3 August 2023: Nagoya), 38th International Cosmic Ray Conference, ICRC 2023, Pos proceedings of science (444), 1043
Publication Publié, 2024-03-01
Publication dans des actes
| Résumé : | 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 -100 m 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. |
