activity
20172021
most citedA -ray Quasi-Periodic modulation in the Blazar PKS 0301243?

54 citations · 128 across the 3 of their papers we have counts for

collaborators

10 papers

astro-ph.HE202132 cited

A Quasi-periodic Oscillation in the gamma-ray Emission from the Non-blazar Active Galactic Nucleus PKS 0521-36

Haiyun Zhang, Dahai Yan, Pengfei Zhang +2

Long-term gamma-ray variability of a non-blazar Active Galactic Nucleus (AGN) PKS 0521-36 is investigated by using Fermi-LAT pass 8 data covering from 2008 August to 2021 March. Th…

astro-ph.HE2021

A Radio Quasi-periodic Oscillation of 176 day in the Radio-loud Narrow-line Seyfert 1 Galaxy J0849+5108

Pengfei Zhang, Zhongxiang Wang

We analyze the 11-year long-term light curve of the Radio-loud Narrow-line Seyfert 1 (NLSy1) galaxy J0849+5108 and the nearly simultaneous -ray data of the source. The data were…

astro-ph.HE202042 cited

Gaussian Process Modeling -LAT -ray Blazar Variability: A Sample of Blazars with -ray Quasi-periodicities

Shenbang Yang, Dahai Yan, Pengfei Zhang +2

Blazar variability may be driven by stochastic processes. On the other hand, quasi-periodic oscillation (QPO) behaviors are recently reported to be detected in -LAT dat…

astro-ph.HE2020

Searching for Quasi-Periodic Modulations in -ray Active Galactic Nuclei

Pengfei Zhang, Dahai Yan, Jianeng Zhou +2

We perform a systematic search of quasi-periodic variabilities in -ray active galactic nuclei (AGNs) in the third \emph{Fermi} Large Area Telescope source catalog (3FGL). We emp…

astro-ph.HE2019

Statistical analysis on X-ray flares from the nucleus and HST-1 knot in the M87 jet

Shenbang Yang, Dahai Yan, Benzhong Dai +4

The statistical properties of X-ray flares from two separate locations (nucleus and HST-1) in the M87 jet are investigated to reveal the physical origin of the flares. We analyse t…

astro-ph.HE2018

Impact of Plasma Instability on Constraint of the Intergalactic Magnetic Field

Dahai Yan, Jianeng Zhou, Pengfei Zhang +2

A relativistic electron-positron pair beam can be produced in the interaction of TeV photons from a blazar with the extragalactic background light (EBL). The relativistic