Search Results - "Barwick, S. W"
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NuRadioMC: simulating the radio emission of neutrinos from interaction to detector
Published in The European physical journal. C, Particles and fields (31-01-2020)“…NuRadioMC is a Monte Carlo framework designed to simulate ultra-high energy neutrino detectors that rely on the radio detection method. This method exploits…”
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New limits on the ultrahigh energy cosmic neutrino flux from the ANITA experiment
Published in Physical review letters (31-07-2009)“…We report initial results of the first flight of the Antarctic Impulsive Transient Antenna (ANITA-1) 2006-2007 Long Duration Balloon flight, which searched for…”
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Constraints on cosmic neutrino fluxes from the Antarctic Impulsive Transient Antenna experiment
Published in Physical review letters (05-05-2006)“…We report new limits on cosmic neutrino fluxes from the test flight of the Antarctic Impulsive Transient Antenna (ANITA) experiment, which completed an 18.4…”
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Cosmic-Ray Electrons and Positrons from 1 to 100 GeV: Measurements with HEAT and Their Interpretation
Published in The Astrophysical journal (20-09-2001)Get full text
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Measurements of the Cosmic-Ray Positron Fraction from 1 to 50 GeV
Published in The Astrophysical journal (20-06-1997)Get full text
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Design and Performance of the ARIANNA HRA-3 Neutrino Detector Systems
Published in IEEE transactions on nuclear science (01-10-2015)“…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 (HRA)…”
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Observation of ultrahigh-energy cosmic rays with the ANITA balloon-borne radio interferometer
Published in Physical review letters (08-10-2010)“…We report the observation of 16 cosmic ray events with a mean energy of 1.5 × 10¹⁹ eV via radio pulses originating from the interaction of the cosmic ray air…”
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The Energy Spectra and Relative Abundances of Electrons and Positrons in the Galactic Cosmic Radiation
Published in The Astrophysical journal (10-05-1998)Get full text
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Observations of the Askaryan effect in ice
Published in Physical review letters (26-10-2007)“…We report on observations of coherent, impulsive radio Cherenkov radiation from electromagnetic showers in solid ice. This is the first observation of the…”
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Optical properties of deep glacial ice at the South Pole
Published in AMANDA-projektet (16-07-2006)“…We have remotely mapped optical scattering and absorption in glacial ice at the South Pole for wavelengths between 313 and 560 nm and depths between 1100 and…”
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Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data
Published in The European physical journal. C, Particles and fields (04-01-2020)“…The Neutrino Mass Ordering (NMO) remains one of the outstanding questions in the field of neutrino physics. One strategy to measure the NMO is to observe…”
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Search for neutrinos from decaying dark matter with IceCube
Published in The European physical journal. C, Particles and fields (16-10-2018)“…With the observation of high-energy astrophysical neutrinos by the IceCube Neutrino Observatory, interest has risen in models of PeV-mass decaying dark matter…”
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Optical Properties of the South Pole Ice at Depths Between 0.8 and 1 Kilometer
Published in Science (American Association for the Advancement of Science) (24-02-1995)“…The optical properties of the ice at the geographical South Pole have been investigated at depths between 0.8 and 1 kilometer. The absorption and scattering…”
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Observation of high-energy neutrinos using Cerenkov detectors embedded deep in Antarctic ice
Published in Nature (London) (22-03-2001)“…Neutrinos are elementary particles that carry no electric charge and have little mass. As they interact only weakly with other particles, they can penetrate…”
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UV and optical light transmission properties in deep ice at the South Pole
Published in Geophysical research letters (01-06-1997)“…Both absorption and scattering of light at wavelengths 410 to 610 nanometers were measured in the South Pole ice at depths 0.8 to 1 kilometer with the laser…”
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Cosmic ray positrons at high energies: A new measurement
Published in Physical review letters (17-07-1995)Get full text
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Cosmic ray reentrant electron albedo: High-Energy Antimatter Telescope balloon measurements from Fort Sumner, New Mexico
Published in Journal of Geophysical Research (01-03-1998)“…The High‐Energy Antimatter Telescope (HEAT) balloon cosmic ray detector flew from Fort Sumner, New Mexico on May 3–5, 1994. The instrument measured electron…”
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Deep-learning-based reconstruction of the neutrino direction and energy for in-ice radio detectors
Published 21-09-2022“…Astroparticle Physics 145 (2023) 102781 Ultra-high-energy (UHE) neutrinos ($>10^{16}$ eV) can be measured cost-effectively using in-ice radio detection, which…”
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Observation of muons using the polar ice cap as a Cerenkov detector
Published in Nature (London) (26-09-1991)“…The need for neutrino telescopes much larger than the detectors now existing is discussed. Research results suggest that a full-scale Antarctic ice detector is…”
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Evidence for neutrino emission from the nearby active galaxy NGC 1068
Published in Science (American Association for the Advancement of Science) (04-11-2022)“…A supermassive black hole, obscured by cosmic dust, powers the nearby active galaxy NGC 1068. Neutrinos, which rarely interact with matter, could provide…”
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