23 citations
- A. Anker2 profiles3
- A. Hallgren2 profiles3 · h 89
- A. Nelles2 profiles3 · h 53
- A. Novikov2 profiles3 · h 24
- C. Persichilli2 profiles3
- D. Besson3 profiles3 · h 42
- G. Gaswint2 profiles3
- I. Plaisier2 profiles3
- J. Tatar2 profiles3 · h 41
- R. Lahmann2 profiles3 · h 54
- S. Kleinfelder3 profiles3 · h 5
- Christian Gläser2
- Friedrich-Alexander-Universität Erlangen-NürnbergDE3 papers
- Irvine UniversityUS3 papers
- Lawrence Berkeley National LaboratoryUS3 papers
- National Taiwan UniversityTW3 papers
- University of California, IrvineUS3 papers
- University of KansasUS3 papers
- Uppsala UniversitySE3 papers
- Whittier CollegeUS3 papers
- National Research Nuclear University MEPhIRU1 paper
3 papers
astro-ph.HE2021★ 11 cited
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…
astro-ph.IM2021★ 13 cited
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…
astro-ph.IM2020★ 23 cited
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…