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Ke-Yao Wu

3 papers hereh-index 215 citations4 works total

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

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE3

identity via Semantic Scholar / OpenAlex

most citedInvestigating the energy distribution of the high-energy particles in the Crab nebula

6 citations · 6 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2024

Likely detection of GeV γ-ray emission from pulsar wind nebula G32.64+0.53 with Fermi-LAT

Yifan Xiao, Keyao Wu, Jun Fang

In this study, we report the likely GeV γ-ray emissions originating from the pulsar PSR J1849-0001's pulsar wind nebula (PWN) G32.64+0.53. Our analysis covers approximately 14.7 ye…

astro-ph.HE2024

Possible GeV gamma-ray emission from the pulsar wind nebula in CTA 1

Liancheng Zhou, Keyao Wu, Yunlu Gong +1

We report a detection of GeV γ-ray emission potentially originating from the pulsar wind nebula in CTA 1 by analyzing about 15 yr of Fermi Large Area Telescope data. By selecting…

astro-ph.HE2021★ 6 cited

Investigating the energy distribution of the high-energy particles in the Crab nebula

Lu Wen, Ke-Yao Wu, Huan Yu +1

The Crab nebula is a prominent pulsar wind nebula (PWN) detected in multiband observations ranging from radio to very high-energy (VHE) γ-rays. Recently, γ-rays with energies a…

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