activity
20242026
collaborators

6 papers

astro-ph.HE2026

Characterizing the origins of gamma-ray variability of the jetted active galactic nuclei observed with the Fermi-LAT

Yongyun Chen, Qiusheng Gu, Junhui Fan +5

We conducted an analysis of gamma-ray variability in a large sample of jetted active galactic nuclei (AGNs) by utilizing archival Fermi-LAT light curves and applying damped random…

astro-ph.HE2026

The cold molecular gas regulates the activity of active galactic nuclei in massive galaxies

Yongyun Chen, Qiusheng Gu, Luis. C Ho +8

The physical quantities that directly regulate AGN feedback in massive galaxies remain poorly understood. Observations of molecular gas surrounding AGNs suggest that this gas serve…

astro-ph.HE2025

The relation between the optical variability timescale, magnetic field of jets and black hole spin in active galactic nuclei

Yongyun Chen, Qiusheng Gu, Junhui Fan +5

We investigate the relationship among the jet magnetic field, black hole spin, black hole mass, Eddington ratio, and optical variability timescales in jetted active galactic nuclei…

astro-ph.HE2025

Observational evidence for a correlation between the magnetic field of jets and star formation rate in host galaxies

Yongyun Chen, Qiusheng Gu, Junhui Fan +4

Accretion supermassive black holes in the center of active galaxies usually produce ``jets''-collimated bipolar outflows of relativistic particles. Magnetic fields near the black h…

astro-ph.HE2024

Constraining the Binarity of Massive Black Holes in the Galactic Center and Some Nearby Galaxies via Pulsar Timing Array Observations of Gravitational Waves

Xiao Guo, Qingjuan Yu, Youjun Lu

Massive black holes (MBHs) exist in the Galactic center (GC) and other nearby galactic nuclei. As natural outcome of galaxy mergers, some MBHs may have a black hole (BH) companion.…

astro-ph.GA2024

Multi-Layer Perceptron for Predicting Galaxy Parameters (MLP-GaP): stellar masses and star formation rates

Xiaotong Guo, Guanwen Fang, Haicheng Feng +1

The large-scale imaging survey will produce massive photometric data in multi-bands for billions of galaxies. Defining strategies to quickly and efficiently extract useful physical…