X. Bi

activity

19992026

most citedMeasurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite

280 citations · 5k across the 158 of their papers we have counts for

collaborators

Showing 2013Show all

3 papers · 1 filter

astro-ph.HE2013★ 86 cited

Pulsar interpretation for the AMS-02 result

Peng-Fei Yin, Zhao-Huan Yu, Qiang Yuan +1

The AMS-02 collaboration has just published a high precision measurement of the cosmic positron fraction $e^{+} / (e^{-} + e^{+})$ , which rises with energy from $\sim 5$ GeV to $\sim 350$ …

astro-ph.HE2013★ 42 cited

Reconcile the AMS-02 positron fraction and Fermi-LAT/HESS total $e^{\pm}$ spectra by the primary electron spectrum hardening

Qiang Yuan, Xiao-Jun Bi

The recently reported positron fraction up to $\sim 350$ GeV by AMS-02 seems to have tension with the total electron/positron spectra detected by Fermi and HESS, for either pulsar…

astro-ph.HE2013★ 72 cited

Implications of the AMS-02 positron fraction in cosmic rays

Qiang Yuan, Xiao-Jun Bi, Guo-Ming Chen +3

The AMS-02 collaboration has just released its first result of the cosmic positron fraction $e^{+} / (e^{-} + e^{+})$ with high precision up to $\sim 350$ GeV. The AMS-02 result shows the sa…

Pulsar interpretation for the AMS-02 result

Reconcile the AMS-02 positron fraction and Fermi-LAT/HESS total e± spectra by the primary electron spectrum hardening

Implications of the AMS-02 positron fraction in cosmic rays

Reconcile the AMS-02 positron fraction and Fermi-LAT/HESS total $e^{\pm}$ spectra by the primary electron spectrum hardening