activity
20172026
most citedUltrahigh-energy Gamma-Ray Radiation from the Crab Pulsar Wind Nebula

19 citations · 76 across the 16 of their papers we have counts for

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Showing astro-ph.HEShow all

14 papers · 1 filter

astro-ph.HE2026

Timing and Spectral Studies of PSR J2022+3842 with NICER and NuSTAR

Jia-Ning Hu, Xiang-Hua Li, Xian-Ao Wang +6

We report on the long-term timing analysis of PSR J2022+3842 using observations from the Neutron Star Interior Composition Explorer (NICER), along with spectral properties derived…

astro-ph.HE2024★ 9 cited

Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

The LHAASO Collaboration, Zhen Cao, Felix Aharonian +315

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass B…

astro-ph.HE2023★ 8 cited

Implications of a Possible Spectral Structure of Cosmic-ray Protons Unveiled by the DAMPE

Lin Nie, Yang Liu, Zejun Jiang

The recent observations revealed that the cosmic-ray (CR) proton spectrum showed a complex structure: the hardening at and softening at . Howeve…

astro-ph.HE2022★ 11 cited

Flux Variations of Cosmic Ray Air Showers Detected by LHAASO-KM2A During a Thunderstorm on 10 June 2021

LHAASO Collaboration, F. Aharonian, Q. An +268

The Large High Altitude Air Shower Observatory (LHAASO) has three sub-arrays, KM2A, WCDA and WFCTA. The flux variations of cosmic ray air showers were studied by analyzing the KM2A…

astro-ph.HE2022★ 19 cited

Ultrahigh-energy Gamma-Ray Radiation from the Crab Pulsar Wind Nebula

Lin Nie, Yang Liu, Zejun Jiang +1

It has been long debated whether the high-energy gamma-ray radiation from the Crab nebula stems from leptonic or hadronic processes. In this work, we investigate the multi-band non…

astro-ph.HE2021

Likely GeV emission from an old Supernova Remnant: SNR G206.9+2.3

Yunchuan Xiang, Zejun Jiang

A novel -ray supernova remnant (SNR) G206.9+2.3 is first reported in this study. We arrived at this conclusion after analyzing 12.4 years of observation data of the Fermi Large…

astro-ph.HE2021

The Likely Counterpart to -Ray Excess from The Northwest Region of Arp 220

Yun-chuan Xiang, Jun-hao Deng, Ze-jun Jiang

The unknown -ray excess in the northwest region of Arp 220 was revisited by analyzing 11.8 years of the \textit{Fermi} Large Area Telescope (\textit{Fermi}-LAT) data in th…

astro-ph.HE2021★ 3 cited

Evaluation of Hadronic Emission in Starburst Galaxies and Star-forming Galaxies

Yun-chuan Xiang, Ze-jun Jiang, Yun-yong Tang

In this work, we reanalyzed 11 years of spectral data from the \textit{Fermi} Large Area Telescope (\textit{Fermi}-LAT) of currently observed starburst galaxies (SBGs) and star-for…

astro-ph.HE2021★ 6 cited

likely Detection of GeV gamma-Ray Emission from the composite supernova remnant COMP G327.1+1.1 with Fermi-LAT

Yunchuan Xiang, Yi Xing, Zejun Jiang

We report the likely GeV -ray emission from the composite supernova remnant (SNR) COMP G327.1+1.1 by analyzing 12.2 years of the \textit{Fermi} Large Area Telescope (\text…

astro-ph.HE2021★ 2 cited

Fermi-LAT Detection of GeV Gamma-Ray Emission from The Highly Asymmetric Shell Supernova Remnant: SNR G317.3-0.2

Yunchuan Xiang, Zejun Jiang, Yunyong Tang

In this paper, we report the first extended GeV -ray emission, at a significant level of 8.13, from the region of the supernova remnant (SNR) SNR G317.3-0.2 by analyzi…

astro-ph.HE2021★ 3 cited

Fermi-LAT detection of GeV -ray emission from Type Ia supernova remnant G272.2-3.2

Yun-Chuan Xiang, Ze-Jun Jiang

A new -ray source with a significance level of approximately 5 was reported in the region of SNR G272.2-3.2, analysing the approximately 12.4 years of observation data from t…

astro-ph.HE2021

Detection of GeV -Ray Emission from supernova remnant SNR G15.9+0.2 with Fermi-LAT

Yunchuan Xiang, Zejun Jiang, Mengyao Tang

We first report GeV -ray emission from supernova remnant (SNR) G15.9+0.2 in this work. The results show that its power-law spectral index is 2.940.25 with a 6.47 signifi…

astro-ph.HE2020★ 13 cited

Prospects for a Multi-TeV Gamma-ray Sky Survey with the LHAASO Water Cherenkov Detector Array

Yingying Guo, Xiaochuan Chang, Hongbo Hu +1

The Water Cherenkov Detector Array (WCDA) is a major component of the Large High Altitude Air Shower Array Observatory (LHAASO), a new generation cosmic-ray experiment with unprece…

astro-ph.HE2017

A possible explanation of the knee of cosmic light component spectrum from 100 TeV to 3 PeV

Wen-Hui Lin, Bi-Wen Bao, Ze-Jun Jiang +1

The mixed Hydrogen and Helium (H + He) spectrum with a clear steepening at TeV has been detected by ARGO-YBJ experiments. In this paper, we demonstrate that the observed…