538 citations · 1k across the 20 of their papers we have counts for
24 papers
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…
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…
Developing New Analysis Tools for Near Surface Radio-based Neutrino Detectors
ARIANNA Collaboration, A. Anker, P. Baldi +22
The ARIANNA experiment is an Askaryan radio detector designed to measure high-energy neutrino induced cascades within the Antarctic ice. Ultra-high-energy neutrinos above …
Precision measurement of the index of refraction of deep glacial ice at radio frequencies at Summit Station, Greenland
J. A. Aguilar, P. Allison, D. Besson +71
Glacial ice is used as a target material for the detection of ultra-high energy neutrinos, by measuring the radio signals that are emitted when those neutrinos interact in the ice.…
Reconstructing the arrival direction of neutrinos in deep in-ice radio detectors
Ilse Plaisier, Sjoerd Bouma, Anna Nelles
In-ice radio detectors are a promising tool for the discovery of EeV neutrinos. For astrophysics, the implications of such a discovery will rely on the reconstruction of the neutri…
Radiofrequency Ice Dielectric Measurements at Summit Station, Greenland
J. A. Aguilar, P. Allison, D. Besson +65
We recently reported on the radio-frequency attenuation length of cold polar ice at Summit Station, Greenland, based on bistatic radar measurements of radio-frequency bedrock echo…
TAROGE-M: Radio Antenna Array on Antarctic High Mountain for Detecting Near-Horizontal Ultra-High Energy Air Showers
TAROGE Collaboration, Shih-Hao Wang, Jiwoo Nam +45
TAROGE-M is a self-triggered radio antenna array atop the 2700 m high Mt. Melbourne in Antarctica, designed to detect impulsive geomagnetic emission from extensive air showers indu…
In situ, broadband measurement of the radio frequency attenuation length at Summit Station, Greenland
J. A. Aguilar, P. Allison, J. J. Beatty +58
Over the last 25 years, radiowave detection of neutrino-generated signals, using cold polar ice as the neutrino target, has emerged as perhaps the most promising technique for dete…
Measuring the Polarization Reconstruction Resolution of the ARIANNA Neutrino Detector with Cosmic Rays
ARIANNA Collaboration, A. Anker, P. Baldi +30
The ARIANNA detector is designed to detect neutrinos with energies above eV. Due to the similarities in generated radio signals, cosmic rays are often used as test beams f…
Improving sensitivity of the ARIANNA detector by rejecting thermal noise with deep learning
ARIANNA Collaboration, A. Anker, P. Baldi +30
The ARIANNA experiment is an Askaryan detector designed to record radio signals induced by neutrino interactions in the Antarctic ice. Because of the low neutrino flux at high ener…
A next-generation optical sensor for IceCube-Gen2
Vedant Basu, Aya Ishihara, Markus Dittmer +1
For the in-ice component of the next generation neutrino observatory at the South Pole, IceCube-Gen2, a new sensor module is being developed, which is an evolution of the D-Egg and…
The IceCube-Gen2 Collaboration -- Contributions to the 37th International Cosmic Ray Conference (ICRC2021)
Gen2 Collaboration, R. Abbasi, M. Ackermann +437
IceCube-Gen2 is a planned extension of the IceCube Neutrino Observatory at the South Pole. The extension is optimized to search for sources of astrophysical neutrinos from TeV to E…
Reconstructing the neutrino energy for in-ice radio detectors
J. A. Aguilar, P. Allison, J. J. Beatty +56
Starting in summer 2021, the Radio Neutrino Observatory in Greenland (RNO-G) will search for astrophysical neutrinos at energies >10 PeV by detecting the radio emission from partic…
Triboelectric Backgrounds to radio-based UHE Neutrino Exeperiments
J. A. Aguilar, A. Anker, P. Allison +114
The proposed IceCube-Gen2 (ICG2) seeks to instrument ~500 sq. km of Antarctic ice near the geographic South Pole with radio antennas, in order to observe the highest energy (E>1 Ee…
Design and Sensitivity of the Radio Neutrino Observatory in Greenland (RNO-G)
J. A. Aguilar, P. Allison, J. J. Beatty +52
This article presents the design of the Radio Neutrino Observatory Greenland (RNO-G) and discusses its scientific prospects. Using an array of radio sensors, RNO-G seeks to measure…
IceCube-Gen2: The Window to the Extreme Universe
Gen2 Collaboration, M. G. Aartsen, R. Abbasi +431
The observation of electromagnetic radiation from radio to -ray wavelengths has provided a wealth of information about the universe. However, at PeV (10 eV) energies and…
Probing the angular and polarization reconstruction of the ARIANNA detector at the South Pole
ARIANNA Collaboration, A. Anker, S. W. Barwick +22
The sources of ultra-high energy (UHE) cosmic rays, which can have energies up to 10^20 eV, remain a mystery. UHE neutrinos may provide important clues to understanding the nature…
White Paper: ARIANNA-200 high energy neutrino telescope
A. Anker, P. Baldi, S. W. Barwick +33
The proposed ARIANNA-200 neutrino detector, located at sea-level on the Ross Ice Shelf, Antarctica, consists of 200 autonomous and independent detector stations separated by 1 kilo…
Neutrino astronomy with the next generation IceCube Neutrino Observatory
M. G. Aartsen, M. Ackermann, J. Adams +399
The past decade has welcomed the emergence of cosmic neutrinos as a new messenger to explore the most extreme environments of the universe. The discovery measurement of cosmic neut…
Neutrino vertex reconstruction with in-ice radio detectors using surface reflections and implications for the neutrino energy resolution
A. Anker, S. W. Barwick, H. Bernhoff +24
Ultra high energy neutrinos (eV are efficiently measured via radio signals following a neutrino interaction in ice. An antenna placed (15 m) below t…
A search for cosmogenic neutrinos with the ARIANNA test bed using 4.5 years of data
A. Anker, S. W. Barwick, H. Bernhoff +23
The primary mission of the ARIANNA ultra-high energy neutrino telescope is to uncover astrophysical sources of neutrinos with energies greater than . A pilot ar…
The Next-Generation Radio Neutrino Observatory -- Multi-Messenger Neutrino Astrophysics at Extreme Energies
J. A. Aguilar, P. Allison, S. Archambault +58
RNO is the mid-scale discovery instrument designed to make the first observation of neutrinos from the cosmos at extreme energies, with sensitivity well beyond current instrument c…
NuRadioMC: Simulating the radio emission of neutrinos from interaction to detector
Christian Glaser, Daniel García-Fernández, Anna Nelles +24
NuRadioMC is a Monte Carlo framework designed to simulate ultra-high energy neutrino detectors that rely on the radio detection method. This method exploits the radio emission gene…
NuRadioReco: A reconstruction framework for radio neutrino detectors
Christian Glaser, Anna Nelles, Ilse Plaisier +6
While the radio detection of cosmic rays has advanced to a standard method in astroparticle physics, the radio detection of neutrinos is just about to start its full bloom. The suc…