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20112023
most citedEvidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

1.6k citations · 20.3k across the 175 of their papers we have counts for

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137 papers · 1 filter

astro-ph.HE2023

Search for high-energy neutrinos from magnetars with IceCube

Ava Ghadimi, Marcos Santander

Neutron stars with very strong magnetic fields are known as magnetars. There are multiple theories that predict magnetars may be able to emit high-energy (HE) neutrinos through had…

astro-ph.HE2023★ 1 cited

The IceCube-Gen2 Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023)

IceCube-Gen2, :, R. Abbasi +452

IceCube-Gen2 is a planned next-generation neutrino observatory at the South Pole that builds upon the successful design of IceCube. Integrating two complementary detection technolo…

astro-ph.HE2023★ 307 cited

Observation of high-energy neutrinos from the Galactic plane

R. Abbasi, M. Ackermann, J. Adams +385

The origin of high-energy cosmic rays, atomic nuclei that continuously impact Earth's atmosphere, has been a mystery for over a century. Due to deflection in interstellar magnetic…

astro-ph.HE2022★ 485 cited

Evidence for neutrino emission from the nearby active galaxy NGC 1068

IceCube Collaboration, R. Abbasi, M. Ackermann +382

We report three searches for high energy neutrino emission from astrophysical objects using data recorded with IceCube between 2011 and 2020. Improvements over previous work includ…

astro-ph.HE2022★ 65 cited

Searches for Neutrinos from Gamma-Ray Bursts using the IceCube Neutrino Observatory

R. Abbasi, M. Ackermann, J. Adams +378

Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs) due to their large power output. Observing a neutrino flux from GRBs would off…

astro-ph.HE2022★ 19 cited

Searching for High-Energy Neutrino Emission from Galaxy Clusters with IceCube

R. Abbasi, M. Ackermann, J. Adams +378

Galaxy clusters have the potential to accelerate cosmic rays (CRs) to ultra-high energies via accretion shocks or embedded CR acceleration sites. CRs with energies below the Hillas…