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researcher

Hao Wang

3 papers hereh-index 113 citations3 works total

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

author position
  • first author2
  • middle author1

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

fields
  • astro-ph.HE3
same name
  • Hao Wang — 33 papers, h 13
  • Hao Wang — 31 papers, h 101
  • Hao Wang — 31 papers
  • Hao Wang — 25 papers, h 18
  • Hao Wang — 24 papers, h 7
  • Hao Wang — 22 papers, h 8

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
20232025
most citedConstraining the long-lived supramassive neutron stars by magnetar boosted kilonovae

18 citations · 19 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 1 cited

EP241217a: a likely Type II GRB with an achromatic bump at z = 4.59

Hao Zhou, Jia Ren, Chen-Wei Wang +22

EP241217a is an X-ray transient detected by the Einstein Probe (EP) lasting for about 100 seconds and without accompanying γ-ray detection. The optical spectroscopy reveals the r…

astro-ph.HE2024

jetsimpy: A Highly Efficient Hydrodynamic Code for Gamma-ray Burst Afterglow

Hao Wang, Ranadeep G. Dastidar, Dimitrios Giannios +1

Gamma-ray burst (GRB) afterglows are emissions from ultrarelativistic blast waves produced by a narrow jet interacting with surrounding matter. Since the first multimessenger obser…

astro-ph.HE2023★ 18 cited

Constraining the long-lived supramassive neutron stars by magnetar boosted kilonovae

Hao Wang, Paz Beniamini, Dimitrios Giannios

Kilonovae are optical transients following the merger of neutron star binaries, which are powered by the r-process heating of merger ejecta. However, if a merger remnant is a long-…

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