823 citations · 2.1k across the 21 of their papers we have counts for
10 papers · 1 filter
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…
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 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…
Targeting ultra-high energy neutrinos with the ARIANNA experiment
A. Anker, S. W. Barwick, H. Bernhoff +20
The measurement of ultra-high energy (UHE) neutrinos (E \SI{e16}{eV}) opens a new field of astronomy with the potential to reveal the sources of ultra-high energy cosmic rays e…
Observation of classically `forbidden' electromagnetic wave propagation and implications for neutrino detection
S. W. Barwick, E. C. Berg, D. Z. Besson +16
Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neut…
The IceCube Neutrino Observatory: Instrumentation and Online Systems
IceCube Collaboration, M. G. Aartsen, M. Ackermann +350
The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detect…
Radio detection of air showers with the ARIANNA experiment on the Ross Ice Shelf
S. W. Barwick, D. Z. Besson, A. Burgman +15
The ARIANNA hexagonal radio array (HRA) is an experiment in its pilot phase designed to detect cosmogenic neutrinos of energies above 10^16 eV. The most neutrino-like background st…
Design and Performance of the ARIANNA Hexagonal Radio Array Systems
S. W. Barwick, E. C. Berg, D. Z. Besson +16
We report on the development, installation and operation of the first three of seven stations deployed at the ARIANNA site's pilot Hexagonal Radio Array in Antarctica. The primary…
Radar Absorption, Basal Reflection, Thickness, and Polarization Measurements from the Ross Ice Shelf
S. W. Barwick, E. C. Berg, D. Besson +10
Radio-glaciological parameters from Moore's Bay, in the Ross Ice Shelf, have been measured. The thickness of the ice shelf in Moore's Bay was measured from reflection times of radi…
Time Domain Response of the ARIANNA Detector
S. W. Barwick, E. C. Berg, D. Z. Besson +12
The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino int…