collaborators

6 papers

astro-ph.HE2026

Utilizing Dispersion Measure of Fast Radio Bursts to Probe the Intergalactic Medium Turbulence

Rui-Nan Li, Zhao Joseph Zhang, Kentaro Nagamine +3

Extragalactic fast radio bursts (FRBs) have emerged as powerful probes of turbulence within the intergalactic medium (IGM), a phenomenon that plays a crucial role in various cosmol…

astro-ph.HE2026

Accretion-Mode Transition: The Driver Behind Spectral Changes in Changing-Look AGNs

Pengyuan Han, Huaiyuan Lu, Bing Lyu +2

The physical origin of optical changing-look AGNs (CLAGNs), characterized by the appearance or disappearance of broad emission lines, is thought to be mainly driven by the variatio…

astro-ph.HE2026

A Universal 1.5 GeV Gamma-Ray Line in Active Galactic Nuclei

Shi-Ju Kang, Yue Yin, Yong-Gang Zheng +1

We report the detection of a gamma-ray spectral line at approximately 1.5 GeV in three active galactic nuclei (AGN) using 17 years of Fermi-LAT observations. The sample includes bo…

astro-ph.HE2026

Locating the missing large-scale emission in the jet of M87* with short EHT baselines

Boris Georgiev, Paul Tiede, Sebastiano D. von Fellenberg +280

In Very-Long Baseline Interferometric arrays, nearly co-located stations probe the largest scales and typically cannot resolve the observed source. In the absence of large-scale st…

astro-ph.HE2024

Hunting for the candidates of Changing-Look Blazar using Mclust Clustering Analysis

Shi-Ju Kang, Shan-Shan Ren, Yong-Gang Zheng +1

The changing-look blazars (CLBs) are the blazars that their optical spectral lines at different epochs show a significant changes and present a clear transition between the standar…

astro-ph.HE2024

The changing-look AGN SDSS J101152.98+544206.4 is returning to a type I state

Bing Lyu, Xue-Bing Wu, Yuxuan Pang +11

Aims. We reported the discovery that a changing-look AGN SDSS J101152.98+544206.4 (J1011+5442 for short) gradually returns to the type 1 state after a short period between 2014 and…