activity
20152026
most citedWhat drives the velocity dispersion of ionized gas in star-forming galaxies?

37 citations · 138 across the 33 of their papers we have counts for

collaborators

34 papers

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

Radio-Gamma-Ray Properties and High-Energy Implications for Fermi Blazars

Xu-Hong Ye, Wen-Xin Yang, Guo-Hai Chen +5

Radio and -ray emissions in blazars, a subclass of active galactic nuclei (AGNs), provide important insight into their high-energy radiation processes. We studied the relation b…

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

A universal relationship between the variability timescale and black hole mass in black hole jetted and non-jetted accreting systems

Yongyun Chen, Qiusheng Gu, Junhui Fan +4

A long-term variability study spanning a range of black hole mass systems, from microquasars hosting stellar-mass black holes to active galactic nuclei (AGNs) harboring supermassiv…

astro-ph.GA2026★ 1 cited

Identifying Compton-thick active galactic nuclei in the COSMOS. II. Searching among mid-infrared selected AGNs

Xiaotong Guo, Qiusheng Gu, Guanwen Fang +7

Compton-thick active galactic nuclei (CT-AGNs), defined by column density , are so heavily absorbed that their X-ray e…

astro-ph.GA2025

Identifying Compton-thick AGNs with Machine learning algorithm in Chandra Deep Field-South

Rui Zhang, Xiaotong Guo, Qiusheng Gu +7

Compton-thick active galactic nuclei (CT-AGNs), which are defined by column density , emit feeble X-ray radiation, eve…

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★ 3 cited

The Accretion Properties and Jet Mechanisms for the Low-Excitation Radio Galaxies

Xu-Hong Ye, Ranieri D. Baldi, Yong-Yun Chen +2

Radio galaxies (RGs) are a subclass of active galactic nuclei, which are suggested to be the parent populations of blazars. According to the accretion-ejection paragram, RGs can be…

astro-ph.HE2025

The relation between black hole spin, star formation rate, and black hole mass for supermassive black holes

Yongyun Chen, Qiusheng Gu, Junhui Fan +4

Both theoretical models and observational evidence indicate that jets and/or outflows driven by central active supermassive black holes exert a significant feedback effect on the o…

astro-ph.HE2025

The relation between black hole spin and star formation in massive star-forming galaxies

Yongyun Chen, Qiusheng Gu, Junhui Fan +4

It has always been believed that feedback from active galactic nuclei (AGN) has an important impact on star formation in massive galaxies. Black hole spin is an important physical…

astro-ph.GA2025

Identifying Compton-thick AGNs in the COSMOS. I. Among X-ray AGNs with Low Photon Counts

Xiaotong Guo, Qiusheng Gu, Guanwen Fang +4

Compton-thick active galactic nuclei (CT-AGNs), characterized by a significant absorption with column densities of , emi…

astro-ph.HE2024★ 4 cited

The Study of Jet Formation Mechanism in Fermi Blazars

Shangchun Xie, Zhihao Ouyang, Jingyu Wu +5

The origin of jet launching mainly comes from two mechanisms: the BZ mechanism and the BP mechanism. However, it is in debate which one is dominating in blazars. In this work, we u…

astro-ph.HE2024

The relation between black hole spin and molecular gas in massive galaxies

Chen Yongyun, Gu Qiusheng, Fan Junhui +4

Molecular gas is the key probe for the complex interaction between the accretion of black holes and star formation of the host galaxy of active galactic nuclei (AGN). The molecular…

astro-ph.HE2024

Jets, accretion and spin in supermassive black holes

Yongyun Chen, Qiusheng Gu, Jianghe Yang +5

The theoretical model suggests that relativistic jets of AGN rely on the black hole spin and/or accretion. We study the relationship between jet, accretion, and spin using supermas…

astro-ph.HE2024

A Minimal Stochastic Variability Model of Blazars in Turbulent Cascade

Nan Ding, Yunyong Tang, Qiusheng Gu +2

In this paper, we propose a novel minimal physical model to elucidate the long-term stochastic variability of blazars. The model is built on the realistic background of magnetized…

astro-ph.HE2023

Jet power extracted from ADAFs and the application to Fermi BL Lacertae objects

Chen Yongyun, Gu Qiusheng, Fan Junhui +4

We calculate the jet power of the Blandford-Znajek (BZ) model and the hybrid model based on the self-similar solution of advection-dominated accretion flows (ADAFs). We study the f…

astro-ph.HE2023★ 3 cited

The comparison of optical variability of broad-line Seyfert 1 and narrow-line Seyfert 1 galaxies from the view of Pan-STARRS

Hongtao Wang, Chao Guo, Hongmin Cao +3

By means of the data sets of the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS), we investigate the relationship between the variability amplitude and luminosity…

astro-ph.HE2023

General Physical Properties of Fermi blazars

Yongyun Chen, Qiusheng Gu, Junhui Fan +6

We study the general physical properties of Fermi blazars using the Fermi fourth source catalog data (4FGL-DR2). The quasi-simultaneous multiwavelength data of Fermi blazar are fit…

astro-ph.HE2023★ 11 cited

General Physical Properties of Gamma-Ray-emitting Radio Galaxies

Yongyun Chen, Qiusheng Gu, Junhui Fan +4

We study the radio galaxies with known redshift detected by the Fermi satellite after 10 years of data (4FGL-DR2). We use a one-zone leptonic model to fit the quasi-simultaneous mu…

astro-ph.HE2023

Curvature of the spectral energy distribution, Compton dominance and synchrotron peak frequency in jetted AGNs

Chen Yongyun, Gu Qiusheng, Fan Junhui +4

We collect a large sample with a reliable redshift detected by the Fermi satellite after 10 years of data (4FGL-DR2), including blazars, -ray Narrow-line Seyfert 1 galaxies (…

astro-ph.HE2023

Jet power, intrinsic -ray luminosity and accretion in jetted AGN

Chen Yonhyun, Gu Qiusheng, Fan Junhui +4

The correlation between the kinetic jet power , intrinsic -ray luminosity () and accretion () may reveal the underlying jet physics in va…

astro-ph.GA2023★ 3 cited

Multiwavelength Analysis of a Nearby Heavily Obscured AGN in NGC 449

Xiaotong Guo, Qiusheng Gu, Jun Xu +5

We presented the multiwavelength analysis of a heavily obscured active galactic nucleus (AGN) in NGC 449. We first constructed a broadband X-ray spectrum using the latest NuSTAR an…

astro-ph.HE2022

The jet formation mechanism of Gamma-ray Narrow-line Seyfert 1 Galaxies

Chen Yongyun, Gu Qiusheng, Fan Junhui +4

Under the coronal magnetic field, we estimate the maximal jet power of the Blandford-\Znajek (BZ) mechanism, Blandford-\Payne (BP) mechanism, and hybrid model. The jet power of the…

astro-ph.GA2022★ 4 cited

The Variability of the Narrow-line Seyfert 1 Galaxies from the PanSTARRS's View

Hongtao Wang, Yanping Su, Xue Ge +2

By means of the data sets from the Pan-STARRAS1 survey, we have systematically examined the relationship between the variability characteristics and the physical parameters of the…