activity
20242026
most citedProperties and Possible Physical Origins of -ray Emission in Extreme Synchrotron Blazars

1 citations · 1 across the 5 of their papers we have counts for

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8 papers

astro-ph.HE2026

Searching for -ray emission from a bona fide Compact Symmetric Object sample: a -ray signal near GB6 J0906+4124

Ying-Ying Gan, Kai Wang, Ji-Shun Lian +1

As a particular subclass of active galactic nuclei (AGNs), compact symmetric objects (CSOs) have attracted significant attention due to potential role as young AGNs. Several -r…

astro-ph.HE2026

Fast Optical Variability of the TeV Blazar PKS 1725+123 Observed by SVOM-VT and Insights from Multi-wavelength Follow-up Observations

Shuo-Yu Liu, Yu-Wei Yu, Ji-Shun Lian +29

PKS 1725+123 is a flat-spectrum radio quasar (FSRQ) with a redshift of . The detection of this object in the TeV band was reported by the MAGIC telescopes and H.E.S.S. in…

astro-ph.HE2026

Spectral Variations of -rays in Mrk 421

Rui-Qi Huang, Xin-Ke Hu, Yu-Wei Yu +2

We present a comprehensive analysis of the 17-year Fermi-LAT observational data of Mrk 421 to investigate the spectral variations in the -ray bands. The light curve of the sour…

astro-ph.HE20261 cited

Properties and Possible Physical Origins of -ray Emission in Extreme Synchrotron Blazars

Ji-Shun Lian, Jia-Xuan Li, Ze-Rui Wang +3

Extreme synchrotron blazars, characterized by a first peak in their broadband spectral energy distributions (SEDs) at frequencies exceeding Hz, often exhibit a second pea…

astro-ph.HE2025

Hadronic Processes in Advection-Dominated Accretion Flow as the Origin of TeV Excesses in BL Lac Objects

Ji-Shun Lian, Ze-Rui Wang, Jin Zhang

The spectral energy distributions (SEDs) of certain BL Lac objects (BL Lacs) exhibit an additional hard -ray component in the TeV energy range that surpasses the predictions of…

astro-ph.HE2025

Two-Component gamma-ray Emission Spectrum and X-Ray Polarization of the Radio Galaxy Pictor A

Jia-Xuan Li, Xin-Ke Hu, Ji-Shun Lian +6

Pictor A is a -ray emitting radio galaxy and has a bright hotspot called WHS, located 4 arcmin away from the nucleus. In this work, we present an analysis of its 16-year…