Origin of Galactic Sub-PeV Diffuse Gamma-Ray Emission: Constraints from High-energy Neutrino Observations
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/2041-8213/ac02c5/pdf
Reference36 articles.
1. Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data
2. Time-Integrated Neutrino Source Searches with 10 Years of IceCube Data
3. HAWC observations of the acceleration of very-high-energy cosmic rays in the Cygnus Cocoon
4. A Very High Energy γ-Ray Survey toward the Cygnus Region of the Galaxy
5. A Cocoon of Freshly Accelerated Cosmic Rays Detected by Fermi in the Cygnus Superbubble
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2. Galactic Diffuse γ-Ray Emission from GeV to PeV Energies in Light of Up-to-date Cosmic-Ray Measurements;The Astrophysical Journal;2023-10-26
3. Measurement of Ultra-High-Energy Diffuse Gamma-Ray Emission of the Galactic Plane from 10 TeV to 1 PeV with LHAASO-KM2A;Physical Review Letters;2023-10-09
4. A dual-zone diffusion model for high energy emissions of the Cygnus Cocoon;Monthly Notices of the Royal Astronomical Society;2023-09-01
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