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Jun-Xian Wang

4 papers hereh-index 310 citations9 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • Jun-Xian Wang — 4 papers
  • Jun-Xian Wang — 1 paper, h 2
  • Jun-Xian Wang — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

collaborators

4 papers

astro-ph.HE2025

A UV to X-Ray View of Soft Excess in Type 1 Active Galactic Nuclei. II. Broadband Correlations

Shi-Jiang Chen, Jun-Xian Wang, Jia-Lai Kang +5

The physical origin of soft X-ray excess (SE) is a long lasting question, with two prevailing theories -- ``warm corona'' and ``ionized reflection'' -- dominating the discussion. I…

astro-ph.HE2025

The Average Soft X-ray Spectra of eROSITA Active Galactic Nuclei

Shi-Jiang Chen, Johannes Buchner, Teng Liu +16

Context. AGNs are strong X-ray emitters shaped by disk-corona interactions. The soft excess (0.5-2.0 keV) reveals key information about the "warm corona" bridging the disk and hot…

astro-ph.HE2025

Disk-jet coupling across the spectral transition in supermassive black holes

Jia-Lai Kang, Chris Done, Scott Hagen +5

Accretion flows in both stellar and supermassive black holes show a distinct spectral transition. This is seen directly in binaries and changing look AGN, and also in a recent samp…

astro-ph.HE2024

A UV to X-ray view of soft excess in type 1 AGNs: I. sample selection and spectral profile

Shi-Jiang Chen, Jun-Xian Wang, Jia-Lai Kang +5

A core sample of 59 unobscured type 1 AGNs with simultaneous XMM-Newton X-ray and UV observations is compiled from archive to probe the nature of soft X-ray excess (SE). In the fir…

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