activity
20242026
collaborators

9 papers

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.GA2025

Possible quasi-periodic optical oscillations of ZTF blazars

Na Wang, Guowei Ren, Shun Zhang +3

Based on the Zwicky Transient Facility (ZTF), we selected 10 blazars as our sample sources. Among these, we found four blazars (J 0923.5+4125, J 1221.3+3010, J 1503.5+4759, and J 1…

astro-ph.GA2025

Baseline-Aware Dependence fitting for DAmping Timescales (BADDAT): A Nearly Unbiased Approach to Constraining Optical Variability Dependence on Physical Properties of Active Galactic Nuclei

Ruisong Xia, Zhen-Yi Cai, Yongquan Xue +7

Active galactic nuclei (AGNs) exhibit stochastic optical variability, commonly characterized by a damped random walk. The damping timescale is of particular interest because it is…

astro-ph.GA2025

A characteristic optical variability time scale in jetted active galactic nuclei: a large gamma-ray emission sample

Dingrong Xiong, Mouyuan Sun, Jun-Xian Wang +14

The variability mechanisms from jetted AGNs are still under debate. Here the damped random walk (DRW) model, implemented through Gaussian Processe (GPs), is used to fit the l…

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.GA2024

How Long Will the Quasar UV/Optical Flickering Be Damped? II. the Observational Test

Guowei Ren, Shuying Zhou, Mouyuan Sun +1

The characteristic timescale at which the variability of active galactic nuclei (AGNs) turns from red noise to white noise can probe the accretion physics around supermassive black…

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…