137 citations · 1.2k across the 70 of their papers we have counts for
12 papers · 2 filters
Macroscopic approach to the radar echo scatter from high-energy particle cascades
E. Huesca Santiago, K. D. de Vries, P. Allison +28
To probe the cosmic particle flux at the highest energies, large volumes of dense material like ice have to be monitored. This can be achieved by exploiting the radio signal. In th…
VAE-based latent-space classification of RNO-G data
Thorsten Glüsenkamp
The Radio Neutrino Observatory in Greenland (RNO-G) is a radio-based ultra-high energy neutrino detector located at Summit Station, Greenland. It is still being constructed, with 7…
Sensitivity of IceCube-Gen2 to measure flavor composition of Astrophysical neutrinos
Neha Lad
The observation of an astrophysical neutrino flux in IceCube and its detection capability to separate between the different neutrino flavors has led IceCube to constraint the flavo…
The next generation neutrino telescope: IceCube-Gen2
Aya Ishihara
The IceCube Neutrino Observatory, a cubic-kilometer-scale neutrino detector at the geographic South Pole, has reached a number of milestones in the field of neutrino astrophysics:…
Performance Studies of the Acoustic Module for the IceCube Upgrade
Charlotte Benning, Jürgen Borowka, Christoph Günther +2
The IceCube Upgrade will augment the existing IceCube Neutrino Observatory by deploying 700 additional optical sensor modules and calibration devices within its center at a depth o…
Benefits of Looking for Coincident Events, Taus, and Muons with the Askaryan Radio Array
Abby Bishop, Austin Cummings, Ryan Krebs +1
Ultra-High Energy (UHE) neutrinos over eV have yet to be observed but the Askaryan Radio Array (ARA) is one in-ice neutrino observatory attempting to make this discovery.…
Multimessenger Potential of the Radio Neutrino Observatory in Greenland
Marco Stein Muzio
The Radio Neutrino Observatory in Greenland (RNO-G) is the only ultrahigh energy (UHE, ~PeV) neutrino monitor of the Northern sky and will soon be the world's most sen…
The Surface Array of IceCube-Gen2
Alan Coleman
The science goals of IceCube-Gen2 include multi-messenger astronomy, astroparticle and particle physics. To this end, the observatory will include several detection methods, includ…
Estimating the coincidence rate between the optical and radio array of IceCube-Gen2
Felix Schlüter, Simona Toscano
The IceCube-Gen2 Neutrino Observatory is proposed to extend the all-flavour energy range of IceCube beyond PeV energies. It will comprise two key components: I) An enlarged 8km…
Deep Learning Based Event Reconstruction for the IceCube-Gen2 Radio Detector
Nils Heyer, Christian Glaser, Thorsten Glüsenkamp
The planned in-ice radio array of IceCube-Gen2 at the South Pole will provide unprecedented sensitivity to ultra-high-energy (UHE) neutrinos in the EeV range. The ability of the de…
Sensitivity of the IceCube-Gen2 Surface Array for Cosmic-Ray Anisotropy Studies
Wenjie Hou
The energy of the transition from Galactic to extra-galactic origin of cosmic rays is one of the major unresolved issues of cosmic-ray physics. However, strong constraints can be o…
The IceCube-Gen2 Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023)
IceCube-Gen2, :, R. Abbasi +452
IceCube-Gen2 is a planned next-generation neutrino observatory at the South Pole that builds upon the successful design of IceCube. Integrating two complementary detection technolo…