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researcher

Wei-hua Wang

4 papers hereh-index 00 citations5 works total

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

author position
  • middle author4

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

fields
  • astro-ph.HE3
  • astro-ph.SR1
same name
  • Wei-Hua Wang — 9 papers, h 19
  • Wei-Hua Wang — 9 papers, h 19
  • Wei-Hua Wang — 8 papers, h 3
  • Wei-Hua Wang — 4 papers, h 22
  • Wei-Hua Wang — 3 papers, h 3
  • Wei-Hua Wang — 2 papers, h 2

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
20242026
most citedThe white-light superflares from cool stars in GWAC triggers

6 citations · 7 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2026

Distinct Modes of Pulsar Glitch Activity Revealed by the Waiting-Time--Amplitude Morphology

Wen-Tong Liu, Wei-hua Wang, Xia Zhou +1

Pulsar glitches display diverse behaviors. They are commonly labeled as "Vela-like" or "Crab-like," yet these qualitative categories do not provide reproducible quantitative bounda…

astro-ph.HE2025

Results of 15-Year Pulsar Timing of PSR J0007+7303 with Fermi-LAT

Zhi-xiang Yu, Shi-jun Dang, Wei-hua Wang +15

The study of pulsar glitches provides a unique window into the internal structure and dynamic processes of neutron stars. PSR J0007+7303, a very bright gamma-ray pulsar, is the fir…

astro-ph.HE2025★ 1 cited

Discovery of the anti-glitch in PSR J1835−1106

Mingyang Wang, Peng Liu, Jianping Yuan +7

We report the detection of an anti-glitch with a fractional frequency change of Δν/ν=−3.46(6)×10−9 in the rotation-powered pulsar PSR J1835−1106 at MJD 55813, based on…

astro-ph.SR2024★ 6 cited

The white-light superflares from cool stars in GWAC triggers

Guang-Wei Li, Liang Wang, Hai-Long Yuan +16

M-type stars are the ones that flare most frequently, but how big their maximum flare energy can reach is still unknown. We present 163 flares from 162 individual M2 through L1-typ…

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