activity
20242026
collaborators

8 papers

astro-ph.HE2026

Circular polarization effects induced by photon-axion mixing in astrophysical environments

Meng Wang, Nan Ding, Qiusheng Gu +2

Axions and axion-like particles (ALPs) are compelling candidates for dark matter and new physics beyond the Standard Model. Photon-axion mixing in external magnetic fields modifies…

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.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…