Particle astrophysics with high energy neutrinos
https://doi.org/10.1016/0370-1573(95)00003-y
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https://doi.org/10.1016/0370-1573(95)00003-y
We use the GALPROP cosmic ray (CR) framework to model the Galactic CR distributions and associated nonthermal diffuse emissions up to PeV energies. We consider ensembles of discrete, finite lifetime CR sources, e.g., supernova remnants, for...
10.3847/1538-4357/adadfb
We present the first X-ray spectropolarimetric results for Cygnus X-1 in its soft state from a campaign of five IXPE observations conducted during 2023 May–June. Companion multiwavelength data during the campaign are likewise shown. The 2–8...
10.3847/2041-8213/ad58e4