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W. Hu

3 papers here

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

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.HE1
same name
  • W. Hu — 35 papers, h 32
  • W. Hu — 12 papers, h 16
  • W. Hu — 5 papers
  • W. Hu — 3 papers, h 11
  • W. Hu — 2 papers, h 5
  • W. Hu — 2 papers, h 3

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

most citedA resolved Lyman-Alpha profile with doubly peaked emission at z~7

1 citations · 1 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025

The origin of X-ray intra-day variability in HBL PKS 2155-304

W. Hu, J. L. Kang, J. X. Wang +2

The origin and physics of X-ray intra-day variability (IDV) in blazars, which is a long-standing issue, is studied by modelling the broad-band X-ray spectrum, the light curves (LCs…

astro-ph.GA2025

Little impact of mergers and galaxy morphology on the production and escape of ionizing photons in the early Universe

S. Mascia, L. Pentericci, M. Llerena +28

Compact, star-forming galaxies with high star formation rate surface densities (ΣSFR​) are often efficient Lyman continuum (LyC) emitters at z≤4.5, likely as inten…

astro-ph.GA2024★ 1 cited

A resolved Lyman-Alpha profile with doubly peaked emission at z~7

C. Moya-Sierralta, J. González-López, L. Infante +7

The epoch of reionization is a landmark in structure formation and galaxy evolution. How it happened is still not clear, especially regarding which population of objects was respon…

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