70 citations · 188 across the 7 of their papers we have counts for
9 papers
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 …
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…
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…
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 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…
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…