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Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
- G. Ambrosi, Q. An, S. Zimmer
- PhysicsNature
- 29 November 2017
TLDR
Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources.
- Z. Cao, F. Aharonian, X. Zuo
- PhysicsNature
- 17 May 2021
TLDR
Possible Dark Matter Annihilation Signal in the AMS-02 Antiproton Data.
- M. Cui, Q. Yuan, Y. S. Tsai, Yi-Zhong Fan
- PhysicsPhysical review letters
- 12 October 2016
TLDR
The Large High Altitude Air Shower Observatory (LHAASO) Science White Paper
- X. Bai, B. Bi, Yunnan University
- Physics
- 7 May 2019
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…
Millisecond pulsar interpretation of the Galactic center gamma-ray excess
- Q. Yuan, Bing Zhang
- Physics
- 8 April 2014
Interpretations of the DAMPE electron data
- Q. Yuan, Lei Feng, Yunlong Zhang
- Physics
- 29 November 2017
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
- Q. Yuan, Xiaoyuan Huang, Siming Liu, Bing Zhang
- Physics
- 19 March 2014
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
- Rui-zhi Yang, Xiao Zhang, Q. Yuan, Siming Liu
- Physics
- 19 May 2014
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…
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