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researcher

J. Wang

4 papers hereh-index 4670 citations12 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 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • J. Wang — 95 papers, h 4
  • J. Wang — 77 papers, h 26
  • J. Wang — 59 papers, h 3
  • J. Wang — 44 papers, h 5
  • J. Wang — 34 papers, h 9
  • J. Wang — 25 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

collaborators

4 papers

astro-ph.HE2026

LHAASO observation of Mrk 421 during 2021 March - 2024 March: a comprehensive VHE catalog of multi-timescale outbursts and its time average behavior

The LHAASO Collaboration, Zhen Cao, F. Aharonian +321

The Large High Altitude Air Shower Observatory (LHAASO) monitors sources within its field of view for up to 7 hours daily, achieving a duty cycle exceeding 98% and an annual point-…

astro-ph.GA2025

An nl-model with a full radiative transfer treatment for level populations of hydrogen atoms in a spherically symmetric H II region

F. -Y. Zhu, J. Wang, Y. Qiu +2

Context. The radiation field consisting of hydrogen recombination lines and continuum emission might significantly affect the hydrogen-level populations in ultra- and hypercompact…

astro-ph.GA2025

MeerKAT view of Hickson Compact Groups:I. Data description and release

R. Ianjamasimanana, L. Verdes-Montenegro, A. Sorgho +25

Context: Hickson Compact Groups (HCGs) are dense gravitationally-bound collections of 4-10 galaxies ideal for studying gas and star formation quenching processes. Aims: We aim to u…

astro-ph.SR2025

Simultaneous existence of the ocsillations, counterstreaming flows and mass injections in solar quiescent prominences

X. L. Yan, Z. K. Xue, J. C. Wang +8

Solar prominences are very spectacular structures embedded in the tenuous and hot solar corona. The counterstreaming flows, a common feature in solar quiescent prominences, have be…

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