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20242026
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astro-ph.HE2026

Revisiting the X-ray Variability Plane of AGNs: The Significant Role of the Photon Index

Ruisong Xia, Hao Liu, Yongquan Xue +9

X-ray variability provides a powerful probe of the innermost regions of active galactic nuclei (AGNs), offering valuable insights into the accretion process and the structure of th…

astro-ph.HE2025

The origin of X-ray intra-day variability in HBL PKS 2155-304

W. Hu, J. L. Kang, J. X. Wang +2

The origin and physics of X-ray intra-day variability (IDV) in blazars, which is a long-standing issue, is studied by modelling the broad-band X-ray spectrum, the light curves (LCs…

astro-ph.HE2024

SMBH binary candidate PKS J2134-0153: Possible multi-band periodic variability and inter-band time lags

Guowei Ren, Mouyuan Sun, Nan Ding +2

Studying the periodic flux-variation behavior of blazars is vital for probing supermassive black hole binaries and the kinematics of relativistic jets. In this work, we report the…

astro-ph.HE2024

Sizes of active galactic nuclei inhomogeneous disks -- large in microlensing, small in reverberation mapping

Guowei Ren, Mouyuan Sun, Jun-Xian Wang +1

Magnetohydrodynamics (MHD) turbulence can drive significant temperature fluctuations in the accretion disk of an active galactic nucleus (AGN). As a result, the disk can be highly…

astro-ph.HE2024

How long will the quasar UV/optical flickering be damped?

Shuying Zhou, Mouyuan Sun, Zhen-Yi Cai +3

The UV/optical light curves of Active Galactic Nuclei (AGNs) are commonly described by the Damped Random Walk (DRW) model. However, the physical interpretation of the damping times…