activity
20172024
most citedA Lyman-α protocluster at redshift 6.9

70 citations · 331 across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2024

Is quasar variability regulated by the close environment of accretion?

Liang Wu, Jun-Xian Wang, Wen-Ke Ren +1

UV/optical variability in quasars is a well-observed phenomenon, yet its primeval origins remain unclear. This study investigates whether the accretion disk turbulence, which is re…

astro-ph.GA2024

A surprising excess of radio emission in extremely stable quasars: a unique clue to jet launching?

Wen-Yong Kang, Jun-Xian Wang, Zhen-Yi Cai +6

Quasars are generally divided into jetted radio-loud and non-jetted radio-quiet ones, but why only 10% quasars are radio loud has been puzzling for decades. Other than jet-induced-…

astro-ph.GA2022★ 8 cited

The Relation between X-ray and Ultraviolet Variability of Quasars

Hao Sou, Jun-Xian Wang, Zhang-Liang Xie +2

The relation between X-ray and UV/optical variability in AGNs has been explored in many individual sources, however a large sample study is yet absent. Through matching the XMM-New…

astro-ph.GA2022★ 6 cited

Exploring the Connection between UV/Optical Variations and Radio Emission in Radio-Quiet Quasars: Clues on Radio Emission Origin

Mai Liao, Junxian Wang, Wenyong Kang +1

The radio emission in radio-quiet quasars (RQQs) has been a long mystery and its physical origin remains unclear. In a previous work we find UV/optical more variable quasars have s…

astro-ph.EP2021★ 56 cited

ExoClock project II: A large-scale integrated study with 180 updated exoplanet ephemerides

A. Kokori, A. Tsiaras, B. Edwards +102

The ExoClock project is an inclusive, integrated, and interactive platform that was developed to monitor the ephemerides of the Ariel targets to increase the mission efficiency. Th…

astro-ph.GA2021★ 11 cited

More variable quasars have stronger emission lines

Wen-Yong Kang, Jun-Xian Wang, Zhen-Yi Cai +1

The UV/optical variation, likely driven by accretion disc turbulence, is a defining characteristic of type 1 active galactic nuclei (AGNs) and quasars. In this work we investigate…