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Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
The direct detection of a spectral break at about 0.9 teraelectronvolts confirms the evidence found by previous indirect measurements, clarifies the behaviour of the CRE spectrum at energies above 1 terAElectronvolt and sheds light on the physical origin of the sub-teraelectronsvolt CREs.
Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources.
The detection of more than 530 photons at energies above 100 teraelectronvolts and up to 1.4 PeV from 12 ultrahigh-energy γ-ray sources with a statistical significance greater than seven standard deviations is reported.
Possible Dark Matter Annihilation Signal in the AMS-02 Antiproton Data.
Using the latest AMS-02 cosmic-ray antiproton flux data, it is found that a dark matter signal is favored and incorporated into the model self-consistently under a Bayesian framework.
The Large High Altitude Air Shower Observatory (LHAASO) Science White Paper
The Large High Altitude Air Shower Observatory (LHAASO) project is a new generation multi-component instrument, to be built at 4410 meters of altitude in the Sichuan province of China, with the aim
Short GRBs: opening angles, local neutron star merger rate and off-axis events for GRB/GW association
The jet breaks in the afterglow lightcurves of short gamma-ray bursts (SGRBs), rarely detected so far, are crucial for estimating the half-opening angles of the ejecta ($\theta_{\rm j}$) and hence
Interpretations of the DAMPE electron data
The DArk Matter Particle Explorer (DAMPE), a high energy cosmic ray and $\gamma$-ray detector in space, has recently reported the new measurement of the total electron plus positron flux between 25
Fermi Large Area Telescope Detection of Supernova Remnant RCW 86
Using 5.4 yr Fermi Large Area Telescope data, we report the detection of GeV. gamma- ray emission from the shell-type supernova remnant RCW 86 (G315.4-2.3) with a significance of similar to 5.1
Fermi Large Area Telescope observations of the supernova remnant HESS J1731-347
Context. HESS J1731-347 has been identified as one of the few TeV-bright shell type supernova remnants (SNRs). These remnants are dominated by nonthermal emission. and the nature of TeV emission has