The sources of the majority of the high-energy astrophysical neutrinos observed with the IceCube neutrino telescope at the South Pole are unknown. So far, only a flaring gamma-ray blazar was compellingly associated with the emission of high-energy neutrinos. However, several studies suggest that the neutrino emission from the gamma-ray blazar population only accounts for a small fraction of the total astrophysical neutrino flux. In this work we probe the production of high-energy neutrinos in the cores of active galactic nuclei (AGN), induced by accelerated cosmic rays in the accretion disk region. We present a likelihood analysis based on eight years of IceCube data, searching for a cumulative neutrino signal from three AGN samples created...
Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs...
The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with ...
We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10(9) GeV, based...
The sources of the majority of the high-energy astrophysical neutrinos observed with the IceCube neu...
Galactic PeVatrons are Galactic sources theorized to accelerate cosmic rays up to PeV in energy. The...
The majority of astrophysical neutrinos have undetermined origins. The IceCube Neutrino Observatory ...
The IceCube Neutrino Observatory has been continuously taking data to search for O(0.5-10) s long ne...
The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for t...
Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the ...
A search for high-energy neutrinos was performed using data collected by the IceCube Neutrino Observ...
The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for t...
We present the first comprehensive search for high-energy neutrino emission from high- and low-mass ...
Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the exi...
We have searched for extremely high energy neutrinos using data taken with the IceCube detector betw...
Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs...
Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs...
The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with ...
We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10(9) GeV, based...
The sources of the majority of the high-energy astrophysical neutrinos observed with the IceCube neu...
Galactic PeVatrons are Galactic sources theorized to accelerate cosmic rays up to PeV in energy. The...
The majority of astrophysical neutrinos have undetermined origins. The IceCube Neutrino Observatory ...
The IceCube Neutrino Observatory has been continuously taking data to search for O(0.5-10) s long ne...
The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for t...
Beginning in 2016, the IceCube Neutrino Observatory has sent out alerts in real time containing the ...
A search for high-energy neutrinos was performed using data collected by the IceCube Neutrino Observ...
The origins of high-energy astrophysical neutrinos remain a mystery despite extensive searches for t...
We present the first comprehensive search for high-energy neutrino emission from high- and low-mass ...
Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the exi...
We have searched for extremely high energy neutrinos using data taken with the IceCube detector betw...
Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs...
Gamma-ray bursts (GRBs) are considered as promising sources of ultra-high-energy cosmic rays (UHECRs...
The existence of diffuse Galactic neutrino production is expected from cosmic-ray interactions with ...
We report constraints on the sources of ultrahigh-energy cosmic rays (UHECRs) above 10(9) GeV, based...