activity
20212026
most citedFaint AGNs Favor Unexpectedly Long Inter-band Time Lags

25 citations · 82 across the 16 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

The Intermediate-Mass Black Hole Reverberation Mapping Project: Scientific Overview and Sample Characteristics

Hengxiao Guo, Jiancheng Wu, Wenwen Zuo +38

Recent discoveries with the James Webb Space Telescope of massive black holes at high redshift have highlighted fundamental questions about black hole seed formation and the coevol…

astro-ph.HE2026

Jet Power, Bulk Lorentz Factor, Black Hole Spin, and Magnetic Field of Accretion Disk in Jetted Active Galactic Nuclei: A Large Gamma-Ray Emission Sample

Dingrong Xiong, Junhui Fan, Feng Yuan +14

We present a catalog of physical parameters for powerful jet-accretion disk-black hole systems in one of the largest samples of gamma-ray emitting jetted active galactic nuclei (AG…

astro-ph.HE2026

X-ray Fourier lag-frequency spectra modulated by stochastic turbulent acceleration in the jets of high-frequency-peaked BL Lac

Guang-Cheng Xiao, Wen Hu, Da-Guo Jiang +4

X-ray interband time lags are key diagnostics of jet physics and are frequently detected in high-frequency peaked BL Lac (HBL) objects at different epochs with various X-ray telesc…

astro-ph.HE2026

X-ray Quasi-Periodic Oscillations in Active Galactic Nuclei and Their Implications for the Changing Look Phenomenon

Mouyuan Sun, Shuying Zhou, Jihong Liu +12

X-ray timing of active galactic nuclei (AGN) provides a unique probe of gas accretion onto supermassive black holes (SMBHs). Quasi-periodic oscillations (QPOs), which trace gas dyn…

astro-ph.GA2025

Discovery of Repeating Transitions in 16 Changing-look Active Galactic Nuclei

Qian Dong, Zhi-Xiang Zhang, Wei-Min Gu +5

The repeating changing-look active galactic nuclei (RCL AGNs) exhibit multiple appearances and disappearances of broad emission lines (BELs), whose underlying mechanism remains a p…

astro-ph.GA2025

Interband Lag Variability in Active Galactic Nuclei across ZTF Data from Multiple Years

Zhen-Bo Su, Zhen-Yi Cai, Hengxiao Guo +2

Interband lags in the optical continua of active galactic nuclei (AGN) have been observed over years of monitoring, yet their physical origins remain unclear. While variable interb…

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.GA2025

A Sandwich Model for Changing-Look AGNs

Qian-Qi Ma, Wei-Min Gu, Zhen-Yi Cai +4

The spectral variability of changing-look active galactic nuclei (CL-AGNs) occurred on timescales of years to tens of years, posing a significant challenge to the standard thin dis…

astro-ph.GA2024

Is quasar variability regulated by the close environment of accretion?

Liang Wu, Jun-Xian Wang, Wen-Ke Ren +1

UV/optical variability in quasars is a well-observed phenomenon, yet its primeval origins remain unclear. This study investigates whether the accretion disk turbulence, which is re…

astro-ph.GA2024★ 4 cited

The Host Galaxy Fluxes of Active Galaxy Nuclei Are Generally Overestimated by the Flux Variation Gradient Method

Minxuan Cai, Zhen Wan, Zhenyi Cai +2

In terms of the variable nature of normal active galaxy nuclei (AGN) and luminous quasars, a so-called flux variation gradient (FVG) method has been widely utilized to estimate the…

astro-ph.GA2024

A surprising excess of radio emission in extremely stable quasars: a unique clue to jet launching?

Wen-Yong Kang, Jun-Xian Wang, Zhen-Yi Cai +6

Quasars are generally divided into jetted radio-loud and non-jetted radio-quiet ones, but why only 10% quasars are radio loud has been puzzling for decades. Other than jet-induced-…

astro-ph.GA2024★ 13 cited

A new timescale-mass scaling for the optical variation of active galactic nuclei across the intermediate-mass to supermassive scales

Zhen-Bo Su, Zhen-Yi Cai, Mouyuan Sun +3

Variability of active galactic nuclei (AGNs) has long been servicing as an essential avenue of exploring the accretion physics of black hole (BH). There are two commonly used metho…

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

Stellar black holes can "stretch'' supermassive black hole accretion disks

Shuying Zhou, Mouyuan Sun, Tong Liu +3

Stellar black holes (sBHs) are widely believed to exist in the accretion disks of active galactic nuclei (AGNs). Previous studies often focus on the transient emission produced by…

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…

astro-ph.GA2023★ 15 cited

How can the optical variation properties of active galactic nuclei be unbiasedly measured?

Xu-Fan Hu, Zhen-Yi Cai, Jun-Xian Wang

The variability of active galactic nuclei (AGNs) is ubiquitous but has not yet been understood. Measuring the optical variation properties of AGNs, such as variation timescale and…

astro-ph.GA2023★ 25 cited

A universal average spectral energy distribution for quasars from optical to extreme ultraviolet

Zhen-Yi Cai, Jun-Xian Wang

The well-known anti-correlation between the optical/ultraviolet (UV) emission line equivalent widths of active galactic nuclei and the continuum luminosity (the so-called Baldwin e…

astro-ph.HE2021★ 25 cited

Faint AGNs Favor Unexpectedly Long Inter-band Time Lags

Ting Li, Mouyuan Sun, Xiaoyu Xu +12

Inconsistent conclusions are obtained from recent active galactic nuclei (AGNs) accretion disk inter-band time-lag measurements. While some works show that the measured time lags a…