2002 - Fellow of American Physical Society (APS) Citation For contributions to nonaccelerator, experimental particle physics, especially as cospokesperson of the Antarctic Muon and Neutrino Detector Array, charged with oversight of detector operations and management of scientific output
His primary areas of investigation include Neutrino, Astrophysics, Cosmic ray, Neutrino detector and IceCube Neutrino Observatory. His studies in Neutrino integrate themes in fields like Astronomy and Muon. His research in Muon focuses on subjects like Astroparticle physics, which are connected to Galaxy.
He combines subjects such as Telescope, Elementary particle, Earth's magnetic field and Anisotropy with his study of Cosmic ray. As a member of one scientific family, he mostly works in the field of Neutrino detector, focusing on Dark matter and, on occasion, Annihilation, Weakly interacting massive particles and Light dark matter. His IceCube Neutrino Observatory study combines topics from a wide range of disciplines, such as Cherenkov radiation, Detector and Glashow resonance.
His main research concerns Neutrino, Astrophysics, Astronomy, Cosmic ray and Neutrino detector. His Neutrino course of study focuses on Muon and Range. His studies link Muon neutrino with Astrophysics.
His Cosmic ray study combines topics in areas such as Positron, Detector and Anisotropy. His study in Neutrino detector is interdisciplinary in nature, drawing from both Massless particle, Solar neutrino and Lepton. S. W. Barwick has researched Sky in several fields, including Angular resolution, Energy, Blazar and Point source.
Neutrino, Astrophysics, IceCube Neutrino Observatory, Astronomy and Cosmic ray are his primary areas of study. His Neutrino research includes elements of Muon and Sky. His Astrophysics study frequently links to adjacent areas such as Coincident.
S. W. Barwick works mostly in the field of Astronomy, limiting it down to concerns involving Cherenkov radiation and, occasionally, Telescope. As a part of the same scientific family, S. W. Barwick mostly works in the field of Cosmic ray, focusing on Detector and, on occasion, ARIANNA Experiment and Radio wave. In his study, Neutrino oscillation is strongly linked to Oscillation, which falls under the umbrella field of Particle physics.
S. W. Barwick mostly deals with Neutrino, Astrophysics, Sky, Muon and Astronomy. The various areas that S. W. Barwick examines in his Neutrino study include Gravitational wave, Fermi Gamma-ray Space Telescope and Supernova. His study on Supernova also encompasses disciplines like
The study incorporates disciplines such as IceCube Neutrino Observatory, Energy and Coincident in addition to Astrophysics. IceCube Neutrino Observatory is a subfield of Particle physics that S. W. Barwick investigates. In general Astronomy, his work in Galaxy is often linked to Scale linking many areas of study.
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Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
M. G. Aartsen;R. Abbasi;Y. Abdou;M. Ackermann.
Science (2013)
Observation of high-energy astrophysical neutrinos in three years of icecube data
M. G. Aartsen;M. Ackermann;J. Adams;J. A. Aguilar.
Physical Review Letters (2014)
First observation of PeV-energy neutrinos with IceCube
M. G. Aartsen;R. Abbasi;Y. Abdou;M. Ackermann.
Physical Review Letters (2013)
Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
Mark Aartsen;Markus Ackermann;Jenni Adams.
Science (2018)
Measurements of the cosmic-ray positron fraction from 1 to 50 geV
S. W. Barwick;J. J. Beatty;A. Bhattacharyya;C. R. Bower.
The Astrophysical Journal (1997)
First year performance of the IceCube neutrino telescope
A. Achterberg;M. Ackermann;J. Adams;J. Ahrens.
Astroparticle Physics (2006)
The IceCube data acquisition system: Signal capture, digitization, and timestamping
R. Abbasi;M. Ackermann;J. Adams;M. Ahlers.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment (2009)
The IceCube Neutrino Observatory: Instrumentation and Online Systems
M.G. Aartsen;M. Ackermann;J. Adams;J.A. Aguilar.
Journal of Instrumentation (2017)
A COMBINED MAXIMUM-LIKELIHOOD ANALYSIS OF THE HIGH-ENERGY ASTROPHYSICAL NEUTRINO FLUX MEASURED WITH ICECUBE
M. G. Aartsen;K. Abraham;M. Ackermann;J. Adams.
The Astrophysical Journal (2015)
Measurements of the Cosmic-Ray Positron Fraction From 1 to 50 GeV
S. W. Barwick;E. Schneider;J. J. Beatty.
arXiv: Astrophysics (1997)
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