activity
20242026
collaborators

13 papers

astro-ph.HE2026

Locating the Production Sites of High-Energy Neutrinos in Blazar Jets

Rui Xue, Yoshiyuki Inoue, Ze-Rui Wang +2

The production sites of high-energy neutrinos in blazar jets remain poorly constrained. In this work, we investigate the physical conditions required for efficient neutrino product…

astro-ph.HE2026

On the maximum neutrino flux of blazars in the one-zone leptohadronic model

Wei-Jian Li, Rui Xue, Ze-Rui Wang +1

The origin of extragalactic high-energy neutrinos remains a major mystery in astrophysics, with blazars as leading candidate sources. The widely adopted one-zone leptohadronic jet…

astro-ph.HE2026

Quasi-Simultaneous Broadband Spectral Energy Distributions of a Sample of Fermi Blazars -- I. Correlation Results

Yi Zhong, Zhujian Wan, Rui Xue +3

Blazars' non-thermal emission shows rapid variability across all wavelengths, so spectral energy distributions (SEDs) built from quasi-simultaneous data are crucial for revealing t…

astro-ph.SR2026

Stochastic Optical Variability and an rms-flux Relation in the Intermediate Polar EP240309a

S. -Y. Wu, Y. -D. Hu, I. Perez-Garcia +18

Magnetic cataclysmic variables provide a natural laboratory for studying how accretion interacts with compact-object magnetospheres and generates stochastic variability. We present…

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.GA2025

Discovery of a Luminosity-dependent Continuum Lag in NGC 4151 from Photometric and Spectroscopic Continuum Reverberation Mapping

Hai-Cheng Feng, Sha-Sha Li, Mouyuan Sun +17

Accretion onto supermassive black holes (SMBHs) powers active galactic nuclei (AGNs) and drives feedback that shapes galaxy evolution. Constraining AGN accretion disk structure is…