activity
20242026
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astro-ph.GA2026

Empirical Near-Infrared Spectral Templates from SPHEREx: Disentangling AGN and Host-Galaxy Emission

Wenke Ren, Hengxiao Guo, Zhenya Zheng +9

SPHEREx conducts the first all-sky near-infrared spectral survey over 0.75-5.0 m, spanning the transition from host-galaxy starlight to AGN-heated torus emission and enabling sp…

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

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.GA2024

Could the inter-band lag of active galactic nucleus vary randomly?

Zhen-Bo Su, Zhen-Yi Cai, Jun-Xian Wang +18

The inter-band lags among the optical broad-band continua of active galactic nuclei (AGNs) have been intensively explored over the past decade. However, the nature of the lags rema…

astro-ph.GA2024

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…