activity
20242026
collaborators

7 papers

astro-ph.HE2026

Constraints on neutrino emission and hadronic flux from 1LHAASO catalog -ray sources

Xue-Rui Ouyang, Yun-Feng Liang, Shi-Long Chen +2

IceCube has detected neutrino emission from the Galactic Plane (GP) at a significance of , though its origin remains uncertain. Utilizing ten years of IceCube muon-track dat…

astro-ph.HE2026

Investigating the correlations between IceCube high-energy neutrinos and Fermi-LAT -ray observations. II

Ming-Xuan Lu, Yun-Feng Liang, Xuerui Ouyang +2

Given that gamma rays with energies larger than TeV are severely absorbed by background radiation fields, for many extragalactic sources, the GeV-TeV gamma-ray observations are the…

astro-ph.HE2026

A neutrino flare candidate potentially associated with X-ray emission from tidal disruption event ATLAS17jrp

Rong-Lan Li, Chengchao Yuan, Hao-Ning He +5

Tidal disruption events (TDEs), in which stars are disrupted by supermassive black holes, have been proposed as potential sources of high-energy neutrinos through hadronic interact…

astro-ph.HE2025

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.HE2025

A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane

Zhen Cao, Felix Aharonian, Yunxiang Bai +312

Ultra-high-energy (UHE), exceeding 100 TeV (10^12 electronvolts), γ-rays manifests extreme particle acceleration in astrophysical sources. Recent observations by γ-ray telescopes…

astro-ph.HE2025

Search for neutrino emission from LHAASO observed Microquasar with IceCube 10-year data

Rong-Lan Li, Hao-Ning He, Da-Ming Wei

The Large High Altitude Air Shower Observatory (LHAASO) has detected ultra-high-energy (UHE; E>100 TeV) gamma-ray emission from five microquasars, suggesting their potential as Gal…