activity
20182026
most citedA two-zone blazar radiation model for "orphan" neutrino flares

42 citations · 231 across the 28 of their papers we have counts for

collaborators

29 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.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.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

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.GA2021★ 3 cited

Observations of cold gas and star formation in dwarf S0 galaxies

Xue Ge, Qiu-Sheng Gu, Ruben Garcıa-Benito +3

Very little work has been done on star formation in dwarf lenticular galaxies (S0s). We present 2D-spectroscopic and millimetre observations made by Centro Astronomico Hispano Alem…

astro-ph.HE2021★ 14 cited

The origin of the soft X-ray excess in the narrow-line Seyfert 1 galaxy SBS 1353+564

Xinpeng Xu, Nan Ding, Qiusheng Gu +2

We present for the first time the timing and spectral analyses for a narrow-line Seyfert 1 galaxy, SBS 1353+564, using \it{XMM-Newton} and \it{Swift} multi-band observations from 2…

astro-ph.HE2021★ 34 cited

Detection of a possible high-confidence radio quasi-periodic oscillation in the BL Lac PKS J2134-0153

Guowei Ren, Nan Ding, Xiong Zhang +5

We have searched quasi-periodic oscillations (QPOs) for BL Lac PKS J2134-0153 in the 15 GHz radio light curve announced by the Owens Valley Radio Observatory 40-m telescope during…

astro-ph.GA2020★ 8 cited

Multi-wavelength Selected Compton-thick AGNs in Chandra Deep Field-South Survey

Xiaotong Guo, Qiusheng Gu, Nan Ding +2

Even in deep X-ray surveys, Compton-thick active galactic nuclei (CT AGNs, ) are difficult to be identified due to X-ray flux…

astro-ph.HE2020★ 9 cited

From the Fermi blazar sequence to the relation between Fermi blazars and gamma-ray Narrow-line Seyfert 1 Galaxies

Yongyun Chen, Qiusheng Gu, Junhui Fan +6

We use the third catalog of blazars detected by Fermi/LAT (3LAC) and gamma-ray Narrow-line Seyfert 1 Galaxies (gamma-NLSy1s) to study the blazar sequence and relationship between t…

astro-ph.HE2020★ 42 cited

A two-zone blazar radiation model for "orphan" neutrino flares

Rui Xue, Ruo-Yu Liu, Ze-Rui Wang +2

In this work, we investigate the 2014-2015 neutrino flare associated with the blazar TXS 0506+056 and a recently discovered muon neutrino event IceCube-200107A in spatial coinciden…

astro-ph.HE2020★ 17 cited

Detection of a high-confidence quasi-periodic oscillation in radio light curve of the high redshift FSRQ PKS J0805-0111

Guo-Wei Ren, Hao-Jing Zhang, Xiong Zhang +5

In this work, we have searched quasi-periodic oscillations (QPOs) in the 15 GHz light curve of the FSRQ PKS J0805-0111 monitored by the Owens Valley Radio Observatory (OVRO) 40 m t…