User:Ramakr18/Extragalactic cosmic ray/Bibliography

Summary of source

 * Transition from galactic to extragalactic cosmic rays
 * Probing the Extragalactic Cosmic-Ray Origin with Gamma-Ray and Neutrino Backgrounds
 * Directional association of TeV to PeV astrophysical neutrinos with radio blazars
 * Observational Evidence for the Origin of High-energy Neutrinos in Parsec-scale Nuclei of Radio-bright Active Galaxies
 * IceCube Data for Neutrino Point-Source Searches Years 2008-2018
 * Acceleration and propagation of ultra-high energy cosmic rays (review article)
 * Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Measurements at Energies above 10^17.8 eV (Auger paper on mass composition)
 * Original Hillas paper (reference for Hillas criterion + historical review)
 * Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
 * Astrophysical sources of high-energy neutrinos in the IceCube era - section on sources
 * Origin of the ankle in the ultra-high energy cosmic ray spectrum and of the extragalactic protons below it
 * Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition Implications
 * Report of the working group on the composition of ultra-high energy cosmic rays
 * Cosmogenic photon and neutrino fluxes in the Auger era - check references for GRB, neutron stars as ECR sources
 * Measurement of the cosmic ray energy spectrum above 2.5e18 eV using the Pierre Auger Observatory
 * Features of the cosmic ray energy spectrum above 2.5e18 using the Pierre Auger Observatory
 * Highlights from the Pierre Auger Observatory
 * Ultra-high-energy cosmic rays and neutrinos from tidal disruptions by massive black holes
 * Gamma-ray and neutrino emissions due to cosmic ray protons accelerated at intracluster shocks in galaxy clusters
 * Cosmic rays in galaxy clusters and their nonthermal emission
 * Hunting for superheavy dark matter with the highest-energy cosmic rays
 * Ultra high energy cosmic rays from super-heavy dark matter in the context of large exposure observatories