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Jianfeng Wu

9 papers hereh-index 345 citations13 works total

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

author position
  • middle author5
  • last author4

Across the 9 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA4
  • astro-ph.HE4
  • astro-ph.SR1
same name
  • Jianfeng Wu — 51 papers, h 20
  • Jianfeng Wu — 6 papers, h 10
  • Jianfeng Wu — 4 papers, h 2
  • Jianfeng Wu — 4 papers, h 3
  • Jianfeng Wu — 3 papers, h 4
  • Jianfeng Wu — 3 papers, h 15

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

activity
20232026
most citedHI Absorption in Low-power Radio AGNs Detected by FAST

5 citations · 5 across the 9 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

4 papers · 1 filter

astro-ph.HE2026

The X-ray Variability of the Ultraluminous X-ray Sources in the NGC 4631 galaxy

Jiashun Chen, Jianfeng Wu, Zikun Lin

We perform a systematic study on the long-term X-ray variability for the five ultraluminous X-ray sources (ULXs) in the NGC 4631 galaxy (X1-X5), using Chandra, XMM-Newton, and Swif…

astro-ph.HE2026

Early results from the SVOM Observatory Science program

A. Coleiro, L. Tao, F. Cangemi +44

We present the organisation and early results from the Observatory Science program of the Space-based multi-band astronomical Variable Objects Monitor (SVOM), based on data collect…

astro-ph.HE2024

The X-ray enhancements of radio-loud quasars at high redshift: New results at z=4 – 7

Zihao Zuo, Shifu Zhu, W. N. Brandt +4

Highly radio-loud quasars (HRLQs; logR>2.5) at z≳4 show apparent enhanced X-ray emission compared to matched HRLQs at lower redshifts, perhaps due to a redshift-depend…

astro-ph.HE2024

The weakness of soft X-ray intensity: possible physical reason for weak line quasars

Jiancheng Wu, Qingwen Wu, Chichuan Jin +8

Weak-line quasars (WLQs) are a notable group of active galactic nuclei (AGNs) that show unusually weak UV lines even though their optical-UV continuum shapes are similar to those o…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.