activity
20132026
most citedA magnetic reconnection origin for the soft X-ray excess in AGN

12 citations · 14 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

Multi-Period Fermi-LAT and LHAASO Constraints on Axion-Like Particles from Mrk 421 via Profile Likelihood with Gaussian Copula Correlation

Longhua Qin, Jiancheng Wang, Chuyuan Yang +9

We present a joint multi-period analysis of axion-like particles (ALPs) using five sets of simultaneous Fermi-LAT and LHAASO observations of the TeV blazar Mrk~421. Photon-ALP osci…

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.IM2026

CosmicWeb-21cm array: A New Radio Observation Array Design for 21cm Cosmology

Jiancheng Wang, Jirong Mao, Xiangming Cheng +10

This paper presents the CosmicWeb-21cm array, a novel radio interferometer designed to overcome the key challenges in 21 cm cosmology. Its core innovations include: (1) a multi-sca…

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.HE2021★ 2 cited

The Origin of The Soft X-Ray Excess in the Seyfert 1.5 Galaxy ESO 362-G18

Xiao-Gu Zhong, Jian-Cheng Wang

We review the Seyfert 1.5 Galaxy ESO 362-G18 for exploring the origin of the soft X-ray excess. The Warm Corona and Relativistic Reflection models are two main scenarios to interpr…

astro-ph.HE2013★ 12 cited

A magnetic reconnection origin for the soft X-ray excess in AGN

Xiaogu Zhong, Jiancheng Wang

We present a new scenario to explain the soft X-ray excess in Active Galactic Nucleus. The magnetic reconnection could happen in a thin layer on the surface of accretion disk. Elec…