activity
20242026
collaborators

8 papers

astro-ph.HE2026

A high-energy neutrino flare associated with nearby bright interacting supernova SN 2021foa

Ming-Xuan Lu, Yun-Feng Liang, Xue-Rui Ouyang +3

While core-collapse supernovae have been widely discussed as potential neutrino sources, definitive observational evidence has remained elusive. In this work, we report evidence of…

astro-ph.HE2026

On the Apparent Correlation between X-ray and Neutrino Luminosities of Active Galactic Nuclei

Jian-Jun Luo, Ming-Xuan Lu, Yun-Feng Liang

Recent studies have reported a linear correlation between the hard X-ray and high-energy neutrino luminosities of active galactic nuclei (AGN), suggesting a possible physical conne…

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 data…

astro-ph.HE2025

SN2023syz and SN2025cbj: Two Type IIn Supernovae Associated with IceCube High-energy Neutrinos

Ming-Xuan Lu, Yun-Feng Liang, Xiang-Gao Wang +1

Type IIn supernovae (SNe IIn) are a subclass of core-collapse SNe in which strong interactions occur between the ejecta and dense circumstellar material, creating ideal conditions…

astro-ph.HE2025

Investigating the Correlation between ZTF Tidal Disruption Events and IceCube High-energy Neutrinos

Ming-Xuan Lu, Yun-Feng Liang, Xiang-Gao Wang +1

Investigating the correlation between the TDE population and IceCube neutrinos could help us better understand whether TDEs could be potential high-energy neutrino emitters. In thi…

astro-ph.HE2024

Evidence for GeV emission of the superluminous supernova SN 2017egm

Shang Li, Yun-Feng Liang, Neng-Hui Liao +2

Superluminous supernovae (SLSNe) are a new class of transients with luminosities times larger than the usual core-collapse supernovae (SNe). Their origin is still unc…