What is he best known for?
The fields of study he is best known for:
- Neutrino
- Electron
- Astronomy
G. W. Sullivan mainly investigates Neutrino, Astrophysics, Cosmic ray, Neutrino detector and Particle physics.
His research on Neutrino frequently links to adjacent areas such as Muon.
His Astrophysics research incorporates themes from Astronomy and Spectral index.
His work deals with themes such as Pion, Active galactic nucleus, Gamma ray, Milagro and Gamma-ray burst, which intersect with Cosmic ray.
He usually deals with Neutrino detector and limits it to topics linked to Dark matter and Annihilation, Weakly interacting massive particles and Light dark matter.
G. W. Sullivan interconnects Particle accelerator, Universe and Antimatter in the investigation of issues within Particle physics.
His most cited work include:
- Observation of high-energy astrophysical neutrinos in three years of icecube data (904 citations)
- First observation of PeV-energy neutrinos with IceCube (585 citations)
- Measurements of the solar neutrino flux from Super-Kamiokande's first 300 days (568 citations)
What are the main themes of his work throughout his whole career to date?
His scientific interests lie mostly in Neutrino, Astrophysics, Astronomy, Neutrino detector and IceCube Neutrino Observatory.
His Neutrino research is under the purview of Particle physics.
He combines subjects such as Massless particle and Lepton with his study of Neutrino detector.
His biological study spans a wide range of topics, including COSMIC cancer database, Galaxy, Detector and Anisotropy.
The various areas that G. W. Sullivan examines in his Muon study include Spectral line and Energy.
His work on Super-Kamiokande as part of general Nuclear physics study is frequently linked to Baseline, therefore connecting diverse disciplines of science.
He most often published in these fields:
- Neutrino (70.54%)
- Astrophysics (53.27%)
- Astronomy (37.50%)
What were the highlights of his more recent work (between 2018-2021)?
- Neutrino (70.54%)
- IceCube Neutrino Observatory (27.38%)
- Astrophysics (53.27%)
In recent papers he was focusing on the following fields of study:
G. W. Sullivan mainly focuses on Neutrino, IceCube Neutrino Observatory, Astrophysics, Astronomy and Cosmic ray.
His Neutrino study results in a more complete grasp of Particle physics.
His IceCube Neutrino Observatory study combines topics in areas such as Meson and Particle acceleration.
His research investigates the link between Astronomy and topics such as Cherenkov radiation that cross with problems in Telescope.
His research in Cosmic ray intersects with topics in Universe and Detector.
G. W. Sullivan has researched Muon in several fields, including Angular resolution, Energy and Muon neutrino.
Between 2018 and 2021, his most popular works were:
- Time-integrated Neutrino Source Searches with 10 years of IceCube Data (72 citations)
- Search for steady point-like sources in the astrophysical muon neutrino flux with 8 years of IceCube data (54 citations)
- Characteristics of the Diffuse Astrophysical Electron and Tau Neutrino Flux with Six Years of IceCube High Energy Cascade Data. (44 citations)
In his most recent research, the most cited papers focused on:
- Electron
- Astronomy
- Neutrino
The scientist’s investigation covers issues in Neutrino, Astrophysics, Astronomy, Sky and IceCube Neutrino Observatory.
The concepts of his Neutrino study are interwoven with issues in Gravitational wave, Supernova, Neutron star and Muon.
G. W. Sullivan has included themes like Light curve, Redshift and Neutrino detector in his Supernova study.
As part of one scientific family, G. W. Sullivan deals mainly with the area of Astrophysics, narrowing it down to issues related to the Energy, and often Gamma-ray burst.
His work in the fields of Astronomy, such as Galaxy and Cosmic ray, overlaps with other areas such as Scale and Context.
IceCube Neutrino Observatory is a primary field of his research addressed under Particle physics.
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