AGN evolution produces the IceCube neutrino spectral break through superposition of contributions from active and post-active phases, with host galaxies acting as efficient cosmic-ray reservoirs.
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KM3NeT reports the first astrophysical neutrino above 100 PeV, reviews tensions with other observatories, and explores source scenarios using the inferred diffuse flux.
A single high-energy neutrino event implies that UHE proton sources must evolve strongly like high-luminosity AGN, but this is disfavored when including null results from other detectors, with proton fraction constrained to about 20% at 20 EeV by composition data.
Spatiotemporal correlation search between IceCube neutrinos and blazar optical flares in expanded samples shows weak signals primarily from two associations, with an upper limit of 8% neutrino contribution from flaring blazars and higher Doppler factors in associated sources.
Minimal UHECR flux models from the Telescope Array predict cosmogenic neutrino fluxes consistent with the KM3-230213A event at the 2σ level.
The MXT data analysis pipeline automatically processes raw X-ray event data into calibrated science products for the SVOM mission's observations of GRBs and transients.
Recent high and ultrahigh energy neutrino detections open a new observational window to the universe by revealing sources and processes inaccessible via photons.
citing papers explorer
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Does the spectral break in the IceCube diffuse neutrino spectrum originate from AGN evolution?
AGN evolution produces the IceCube neutrino spectral break through superposition of contributions from active and post-active phases, with host galaxies acting as efficient cosmic-ray reservoirs.
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KM3-230213A and potential astrophysical sources
KM3NeT reports the first astrophysical neutrino above 100 PeV, reviews tensions with other observatories, and explores source scenarios using the inferred diffuse flux.
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Implications of a Cosmogenic Origin of KM3-230213A for Ultra-High-Energy Protons
A single high-energy neutrino event implies that UHE proton sources must evolve strongly like high-luminosity AGN, but this is disfavored when including null results from other detectors, with proton fraction constrained to about 20% at 20 EeV by composition data.
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Association of the IceCube neutrinos with CAZ blazar light curves
Spatiotemporal correlation search between IceCube neutrinos and blazar optical flares in expanded samples shows weak signals primarily from two associations, with an upper limit of 8% neutrino contribution from flaring blazars and higher Doppler factors in associated sources.
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Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models
Minimal UHECR flux models from the Telescope Array predict cosmogenic neutrino fluxes consistent with the KM3-230213A event at the 2σ level.
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The data analysis pipeline for the Microchannel X-ray Telescope on board the SVOM mission
The MXT data analysis pipeline automatically processes raw X-ray event data into calibrated science products for the SVOM mission's observations of GRBs and transients.
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Particle Astrophysics with High and Ultrahigh Energy Neutrinos
Recent high and ultrahigh energy neutrino detections open a new observational window to the universe by revealing sources and processes inaccessible via photons.